View allAll Photos Tagged NGC3628

If you zoom in you can ever make out Galaxy NGC3628 300,000 light-years long tidal tail off to it's right.

 

Canon EOS 6D (Baader filter modified)

Focal length: Canon 400mm f5.6

Tracking Mount: Skywatcher EM35-Pro.

Guiding: None

Exposure: 100 x 60sec @ ISO-6400 (RAW)

With calibration frames applied.

Software: Astro Pixel Processor & Lightroom.

Object: Leo Triplet (M66 Group)

The Leo Triplet or the M66 Group is a small group of galaxies approximately 35 million light-years away and located in the constellation of Leo. This galaxy group consists of the spiral galaxies M65, M66(NGC3627), and NGC3628 (The Hamburger Galaxy or Sarah’s Galaxy) .

 

-Acquisition Date: 2/22/2020 – 03/01/2020

-Location: Western Massachusetts

-Camera: FLI ML1620 @ -25°C

-Telescope: Astro-TECH AT130 with APM Riccardi APO Flattener 1.0x

-Mount: Astro-Physics AP1100

-Guide scope: Celestron Off Axis Guider

-Guide Camera: ASI174 mini

 

Filters:

Astrodon Gen II E Filters

Luminance: 72 x 120sec (144 min)

Red: 81 x 120sec (162 min)

Green: 72 x 120sec (144 min)

Blue: 78 x 120sec (156 min)

Total Exposure:606 min. (10.1hr)

 

Limiting Magnitude: 5.1

 

Processed in Pixinsight 1.8.8-5 and Adobe PS5

 

Frames recorded at DeepSkyWest with a Takahashi FSQ106EDXIII and QSI683.

 

www.astrobin.com/251880/

 

L: 32x900s

RGB: (12, 13, 15)x600s

 

Copyright: R. Colombari

 

Note: Comet 67P was passing through the field. Its passage is visible near the tidal tail of NGC3628

______________________________

 

Leo Triplet

 

Explanation: A mere 30 million light-years away, large spiral galaxy NGC 3628 (center left) shares its neighborhood in the local Universe with two other large spirals, in a magnificent grouping otherwise known as the Leo Triplet. In fact, fellow trio member M65 is near the center right edge of this deep cosmic group portrait, with M66 just above it and to the left. But, perhaps most intriguing is the spectacular tail stretching down for about 300,000 light-years from NGC 3628's warped, edge-on disk. Known as a tidal tail, the structure has been drawn out of the galaxy by gravitational tides during brief but violent past interactions with its large neighbors. Not often imaged so distinctly, the tidal tail is composed of young bluish star clusters and star-forming regions.

 

Source: APOD

DESCRIPTION: The Leo Triplet, M65, M66, NGC3628, constellation Leo. RA (center) 11h 20 min, DEC 13° 15’, FOV approx 1,9°x 1,3°.

  

GEAR: Nikon Z7 Kolari Full Spectrum + Nikkor 500/5,6 PF, Astronomic UV/IR/L2 Clip in filter, Astroklar light pollution filter, Dew heater strip, tracking mount iOptron CEM60EC

  

ACQUISITION: march 22, 2022, Struz, CZ, Subexposure 180s, f 5,6, ISO 1600, Interval 15 s, RAW-L, Lights 21x, Darks 20x, Bias 20x, Flats 20x, DarkFlats 15x. Total exposure time 63 min. Night, breeze, 3° C, no Moon, Backyard - Light pollution - Bortle 5.

  

STACKING AND POST PROCESSING: AstroPixelProcessor (stacking, background neutralisation, light pollution removal, calibrate background and stars colours), Adobe Photoshop CC 2022 (stretching, black and white point settings, star reduction, enhance DSO, deep space noise reduction, contrast setting and sharpening). Cropped 4,7x, image size 3840 x 2560 px.

 

ASI 294 MC PRO.

72 ED Skywatcher con reductor/aplanador 0.85.

Star Adventurer.

Guiado Asi 120mm Mini.

Ganancia 123/ 30 offset/ -10ºc

41x300s

L-Pro

Bortle 8.

PixInsight, Topaz Denoise AI.

M65 - M66 - NGC 3628: Leo Triplet

 

Optics: Skyrover 130SA 130mm f/5 Refractor

Camera: ZWO ASI6200MM Pro

 

Blue: 42x300 sec

Green: 39x300 sec

Lum: 58x300 sec

Red: 42x300 sec

 

starbase.insightobservatory.com/home

nova.astrometry.net/user_images/11726687#annotated

Calibration

Center (RA, Dec):(169.427, 13.151)

Center (RA, hms):11h 17m 42.536s

Center (Dec, dms):+13° 09' 04.980"

Size:1.91 x 1.56 deg

Radius:1.233 deg

Pixel scale:1.19 arcsec/pixel

 

Tags:

The star n Leo

73 Leo

NGC 3593

NGC 3623

M 65

NGC 3627

M 66

NGC 3628

  

NGC 3628, also known as the Hamburger Galaxy or Sarah's Galaxy, is an unbarred spiral galaxy about 35 million light-years away in the constellation Leo. It was discovered by William Herschel in 1784. It has an approximately 300,000 light-years long tidal tail. Along with M65 and M66, NGC 3628 forms the Leo Triplet, a small group of galaxies. Its most conspicuous feature is the broad and obscuring band of dust located along the outer edge of its spiral arms, effectively transecting the galaxy to the view from Earth.

 

Due to the presence of an x-shaped bulge, visible in multiple wavelengths, it has been argued that NGC 3628 is instead a barred spiral galaxy with the bar seen end-on. Simulations have shown that bars often form in disk galaxies during interactions and mergers, and NGC 3628 is known to be interacting with its two large neighbors.Ngc 3628 Hamburger

 

12 "Truss RC telescope reduced to 1790

Moravian off-axis guider and Moravian G0300 guide camera

Celestron 80/600 guide tube with Asi Zwo 224

Moravian G2 8300 camera with internal wheel

Ioptron Cem120 mount

Moonlite focuser and 3.5 "electronic rotator

Electronic temperature control and anti-condensation bands

Cls ccd, R, G, B, Ha 6nm filters, all Astronomik

 

Shooting data:

 

101x240s Cls CCD

15x600s Ha

31x240s R

31x240s G

31x240s B

 

Processing: Pixinsight, Photoshop, star spikes, astronomy tools

Leo Triplet galaxies (M65, M66 & NGC3628)

L-RGB

Bin1x1 L:2h36mn, Bin2x2 R:21mn, G:30mn & B:18mm exposure time

200/1000 mm Newton telescope

Camera ZWO ASI1600MM Pro

Preprocessing with SIRIL

Image processing with Photoshop

Final touch with Lightroom

"The Leo Triplet, or the M66 Group, is a group of interacting spiral galaxies located in the northern constellation Leo. The group consists of the galaxies Messier 65, Messier 66 and NGC 3628, also known as the Hamburger Galaxy. The Leo Triplet lies at an approximate distance of 35 million light years from Earth."

 

Askar 120APO: 840mm f/7

ZWO ASI533MC Cooled Color Camera at -20C

Guided on ZWO AM5

51x180s with UV/IR cut filter

Processed with PixInsight, Ps

 

NGC 3628, aussi appelé la galaxie du hambuger en raison de ressemblance avec le célèbre sandwich, est une vaste galaxie spirale vue par la tranche et située dans la constellation du Lion à environ 38 millions d'années-lumière de la Voie lactée.

Celestron C9 + ASI1600MC. 120x60s. SIRIL et Photoshop.

Description: The Leo Triplet (also known as the M66 Group) is a small group of galaxies about 35 million light-years away in the constellation Leo. This galaxy group consists of the spiral galaxies NGC 3628 (the edge-on galaxy to the left), M65 (upper right), and M66 (lower right).

 

Equipment:

ZWO ASI6200MM-P/EFW 2" x 7 (LRGB)

TeleVue NP101is/NPR-2073 (4" f/4.3)

Losmandy G11

 

Software:

Captured in NINA

Processed in PixInsight

 

Integration:

L: 137 x 90s = 01:15

R: 36 x 90s = 00:54

G: 40 x 90s = 01:00

B: 40 x 90s = 01:00

Total integration: 4:09.

Last quick pass of the night. A trio of galaxies... M65, M66, and NGC3628. Just an hour of data.... needs about 3-4 hours.

 

NGC3628 is also known as the Hamburger Galaxy and is located in the constellation of Leo about 35 million light years away. Along with M65 and M66 it forms a part of the famous Leo Triplet. It is about 100,000 light years across and has a faint tidal tail about 300,000 light years long, a small portion of which can be seen starting from the upper left corner of the galaxy and extending to the left edge of the screen. it has a prominent dust lane bisecting the main body of the galaxy.

ASI 294 MC PRO.

72 ED Skywatcher con reductor/aplanador 0.85.

Star Adventurer.

Guiado Asi 120mm Mini.

Ganancia 123/ 30 offset/ -10ºc

41x300s

L-Pro

Bortle 8.

PixInsight, Topaz Denoise AI.

Leo Triplet M66-M65-NGC3628 - Galaxies - Constellation Leo The Leo Triplet is composed of the spiral galaxies M66, M65 and NGC3628, they are in interaction with each other and a neutral hydrogen halo connects them, a sign of a close encounter that took place 800 million years ago. The triplet is about 35 million light years from us and is located in the constellation Leo. M66 the largest and brightest of the complex is also known as NGC3627 was discovered by Pierre Méchain in 1780. Quite easy to locate halfway between the stars θ Leonis and ι Leonis. In order to appreciate some of its details, it is necessary to have a telescope with an aperture of at least 150mm. Visible from both hemispheres, the best period for its observation is between February and August. M65 also known as NGC3623 was discovered by Pierre Méchain in 1780 at the same time as M66, Charles Messier described it as a very faint and starless nebula. 22 million light years away from us, it is estimated to have a diameter of about 70,000 light years and a mass equal to 85 billion solar masses. NGC3628 third component of the triplet is less luminous than the others, but very extensive, crossed in its length by a long luminous band, it is about 35 million light years from us, it was discovered in 1784 by William Herschel.

Le fameux trio du Lion au Quattro 20-800. 19 poses de 180s. Siril et Nina. Seccion écourtée cause brouillard.

I tested my new Optolong L Pro filter 77 mm with 70-200/2,8 lens. This photo is only 1 shot - 300 s taken by Nikon Z7, f 2,8, ISO 1600, cropped 15x, FOV 2,7 x 1,8 ang.deg. I could not take more shots because bad weather. I think the result is not bad. Next time I will take more shots including darks, bias and flats. Precessed in Adobe PS + Astronomic tools. Taken on April 22, 2020.

Imaged during the night of the 3-4 March this is an image of the galaxy triplet in the constellation of Leo.

 

Two of the galaxies were catalogued by Charles Messier, M66 (top left) and M65 (bottom left). The third galaxy (right) is found in the NGC Catalogue as NGC 3628.

 

NGC 3628 is popularly known as the "Hamburger Galaxy" due to its edge on appearance to us said to resemble a Hamburger.....!

 

Lying at a distance of 35 million light-years from us they are a true group of interacting systems.

 

Our viewpoint means we see the three galaxies at different angles. NGC appears edge-on - displaying lots of dust and a prominent dust lane.

 

M65 & M66 are inclined enough so that their spiral arms are visible.

 

The three systems are very different in character.

 

M66 is a barred and shows a high rate of star formation with numerous tell-tale red/pink areas of glowing hydrogen gas. Its spiral arms are also deformed, indicative of interactive gravitational forces within the group.

 

M65 is an intermediate spiral and is poor in dust and star formation. It appears the least affected by interaction showing a more or less classical spiral shape.

 

NGC3628 is an unbarred spiral which we see edge on. The galaxy is transacted by a broad band of dust which stretches along its outer edge hiding young stars in the galaxy arms.

 

Imaged with an Esprit 120ED with flattener and a cooled ZWO 2600MC camera.

 

Thanks for looking!

ASI 294 MC PRO.

SV503, 80 ED Svbony con

aplanador x1 (560mm).

HEQ5 PRO.

Guiado Asi 120mm Mini.

Ganancia 123/ Offset 30 -10ºc.

Filtro SV231 (57x300s.)

Bortle 7.

PixInsight.

Captured at PixelSkies, Castillejar, Spain

 

www.pixelskiesastro.com

 

FSQ-85ED details

 

Lum 83 x 600s

Red 49 x 180s

Green 53 x 180s

Blue 49 x 180s

 

21 Hours 23 mins in total.

 

TEC140 details

 

Lum 32x600Secs

 

5 hours 20 mins in total.

 

Equipment used:

 

Telescope: Takahashi Baby Q FSQ-85ED F5.3, TEC140 F7

 

Camera: Xpress Trius SX-694 Pro Mono Cooled to -20C

 

Image Scale: 2.08

 

Guiding: OAG

 

Filters: Astronomik Lum,Red,Green,Blue

 

Mount: iOptron CEM60 "Standard" GOTO Centre Balanced Equatorial Mount

 

Image Acquisition: Voyager

 

Observatory control: Lunatico Dragonfly

 

Stacking and Calibrating: Pixinsight

 

Processing: Pixinsight 1.8, Photoshop CC, StarXTerminator, StarNet v2, NoiseXTerminator, BlurXTerminator

1100mm/F7.3 telescope

Pentax 645z (astro-modified)

Apogee F16M cooled CCD

total exposure time = 34.1 hr

 

see www.astrobin.com/jlmim2/ for more technical details.

2026 Leo Triplet -galaxies M65 M66 NGC3628 with SC_C8+0.63X + ASI533MC-P

Il periodo dell'anno Febbraio-Maggio è chiamato per noi amanti del cielo la "Stagione delle Galassie" poichè è il periodo migliore per osservarle e/o fotografarle.

Questi oggetti del cielo sono generalmente apparentemente piccoli di dimensioni, solo a causa della loro enorme distanza, quindi è preferibile fotografarli con focali medio-lunghe; perciò mi sono nuovamente messo in gioco utilizzando un setup strumentale ai limiti della tolleranza.

A volte le galassie si trovano in gruppi ravvicinati anche se solo prospetticamente. E' il caso del famoso "Tripletto del Leone", formato da 3 galassie molto belle: "M65", "M66" e "NGC3628". Con il mio setup ho dovuto realizzare un mosaico di 2 pannelli e in quasti casi tutto si complica anche a causa dell'Inquinamento Luminoso e delle condizioni meteo non sempre uguali tra le sessioni fotografiche.

Eppure malgrado le difficoltà oggettive ho cercato di raggiungere un dicreto e gradevole risultato e penso di esserci riuscito.

_____________

The period from February to May is known to us sky lovers as "Galaxy Season" because it's the best time to observe and/or photograph them.

These celestial objects are generally seemingly small in size, simply because of their enormous distance, so it's best to photograph them with medium-long focal lengths; so I once again ventured into the unknown, using an instrumental setup at the limits of my capabilities.

Sometimes galaxies are found in close-knit groups, even if only in perspective. This is the case of the famous Leo Triplet, made up of three very beautiful galaxies: "M65", "M66" and "NGC3628". With my setup, I had to create a mosaic of two panels, and in these cases everything gets complicated, also due to light pollution and weather conditions that are not always the same between photographic sessions.

Yet despite the objective difficulties I tried to achieve a decent and pleasant result and I think I succeeded.

_______________

Optic: Celestron SC C8 203mm f/10 + Celestron riducer-corrector 0.63X

Camera: ZWO ASI533MC-Pro

Mount: Sky Watcher HEQ5 Synscan

Seeing: 3 (scala Antoniadi)

Filter: Astronomik CLS

-170+166x180s 250gain/ 23darks /23 flats /80 biases

t° sensor: -10°C

Date: 2026-04-08+09+10+11

Integration: 16h 48m

Temperature: 12°C (media)

location for: Biancavilla -Catania-(Italy) 515m slm (Bortle 5-6) flic.kr/p/8AWHek lightpollutionmap.app/it/?lat=37.641252&lng=14.871604...

Acquisition: NINA, PHDGuiding

Processing: SIRIL1.4.2, GraXpert, SyQon-Prism, SyQon-Starless, PS

 

Date : 2023-02-28

Objet :M65-66 / NGC3628

Instrument : Lunette 80 ED Esprit Super APO Sky_Watcher

Camera : ZWO ASI1600 MC / Filtre = IrCut / Temp = -15°c / Gain= 139 / Offset = 21

Durée pose unitaire = 180s / Nombre de pose : 53

Traitement SIRIL et PHOTOSHOP / Gestion Stellarmate

Equipment:

GSO RC8

1800mm f8

Moravian CCD G2-8300FW10

Astrodon LRGB Filter

Losmandy G11 LFE Photo

 

Guiding:

Starlight Lodestar an Celestron OAG + PHD

 

Date: Januar 2013

M65 - M66 - NGC 3628: Leo Triplet

 

Optics: Skyrover 130SA 130mm f/5 Refractor

Camera: ZWO ASI6200MM Pro

 

Blue: 42x300 sec

Green: 39x300 sec

Lum: 58x300 sec

Red: 42x300 sec

 

starbase.insightobservatory.com/home

nova.astrometry.net/user_images/11726687#annotated

Calibration

Center (RA, Dec):(169.427, 13.151)

Center (RA, hms):11h 17m 42.536s

Center (Dec, dms):+13° 09' 04.980"

Size:1.91 x 1.56 deg

Radius:1.233 deg

Pixel scale:1.19 arcsec/pixel

 

Tags:

The star n Leo

73 Leo

NGC 3593

NGC 3623

M 65

NGC 3627

M 66

NGC 3628

  

ccd: Moravian G3-16200 with EFW + OAG

filters: Optolong LRGB and Astrodon 5-nm Ha/O3

telescope: FSQ 106N f/5

mount: 10Micron GM2000 QCI

guider: Lodestar X2

exposure: L 40x10min + RGB 20x5min (all 1x1)

location: Les Granges, 900 m (Hautes Alpes, France)

software: TheSkyX Pro, CCD Commander, Pixinsight, PS CC

date: 17 - 28 Mar 2020

The Leo Triplet is a group of galaxies (M65, M66, NGC 3628) that are about 35 million lightyears away from us. NGC 3628 (left) is also called the "Hamburger Galaxy".

The image was shot shot from my suburbian balcony (stack of 120 x 180 s ISO 800) with my 130/910mm refractor and a standard Pentax K3ii camera.

Leo Triplet

Credit: Giuseppe Donatiello

 

The Leo Triplet (or M66 Group) is a small group of galaxies at 35 million light-years in Leo. This galaxy group consists of the spiral galaxies M65, M66, and NGC 3628.

M65 11h 18m 56.0s +13° 05′ 32″

Messier 65 (NGC 3623) is an intermediate spiral galaxy and It was discovered by Charles Messier in 1780.

M66 11h 20m 15.0s +12° 59′ 30″

Messier 66 (NGC 3627) is an intermediate spiral galaxy at 36 million light-years. It was also discovered by Charles Messier in 1780.

NGC 3628 11h 20m 17.0s +13° 35′ 23″

NGC 3628, the Hamburger Galaxy is an unbarred spiral galaxy. It was discovered by William Herschel in 1784.

NGC 3628 is an unbarred spiral galaxy in the constellation Leo. This image is a 3 x drizzle crop of my recent image of the Leo Triplet.

 

ASI2600mmp and TS 130/910 mm triplet apo.

 

110 x 90 s luminance

40 x 90 s blue

40 x 90 s green

36 x 90 s red

The Triangulum Galaxy

 

See on Fluidr

 

To see more of my work and to buy prints visit www.jklovelacephotography.com/pages/space

The Leo Triplet or M66 Group. A small galaxy group approximately 35 million light years distant. NGC3628 is at the top left, M65 is on the right and M66 is at the bottom.

 

Luminance imaged from London on the nights of the 29th and 31st March, 4 hours integration consisting of 60 second subs. Luminance only using a Hutech IDAS LPS filter

 

RGB imaged from London on the 11th April 2019,30 minutes integration each colour channel consisting of 30 second subs.

 

TS65 Quad Astrograph and ASI1600MM Pro camera

NGC3628

 

LRGB data from Telescope Live. Processed with PixInsight. Grayscale version.

 

app.telescope.live/en

nova.astrometry.net/user_images/13379326#annotated

Distance 30 Mio. Lj

 

Equipment:

TS 10" f/4 ONTC Newton

1000mm f4

ZWO ASI 1600mmc

Astrodon LRGB

Losmandy G11/LFE Photo

 

Guding:

Lodestar on TS Optics - ultra short 9mm Off Axis Guider

PHD2

 

RGB per 12x120s

Luminanz 60x120s

 

total exposure time: ca. 192 min

 

20.03.2018

 

Processing: PixInsight/CaptureOne

Equipment:

GSO RC8 + CCDT67 Reducer

1100mm f5,5

Moravian CCD G2-8300FW10

Astrodon LRGB Filter

Losmandy G11 LFE Photo

 

Guiding:

Starlight Lodestar an Celestron OAG + PHD

 

Date: Dezember 2014

An attractive grouping of 3 spiral galaxies in Leo about 35 million LY away. Comprising:

 

NGC 3628 “the Hamburger galaxy” - Edge on spiral with prominent dust lane. There is a long tail to the left of the galaxy of stars displaced by a previous gravitational encounter - just visible here.

 

Messier 65 spiral galaxy mostly old stars with little dust or gas except where it may have interacted with the other 2. 1 supernova detected.

 

Messier 66 barred spiral with 5 supernovae detected consistent with excess young Star formation probably due to interaction with the other 2.

 

Astrometry:

Resolution ............... 2.395 arcsec/px

Focal distance ........... 323.84 mm

Pixel size ............... 3.76 um

Field of view ............ 1d 26' 34.5" x 1d 1' 47.3"

Image centre............. RA: 11 20 03.322 Dec: +13 21 05.05

 

System 1 Scope:

Camera: QHY600M 16-Bit CMOS, Binned x2

Optics: Takahashi FSQ130

Aperture: 130mm

Focal Length: 650mm

Focal Ratio: F5

Guiding: Stellarvue 50mm

LeoTriplett, Leo Cluster or Leo Group

 

Distance 35 Mly

 

Equipment:

TS 10" f/4 ONTC Newton

1000mm f4

ZWO ASI 1600mmc

Astrodon LRGB

Losmandy G11/LFE Photo

 

Guding:

Lodestar on TS Optics - ultra short 9mm Off Axis Guider

PHD2

 

M65 M66:

70x120 Lum

RGB 3x12x120s RGB

total exposure time: 212 min

20.02.2018

 

NGC3628:

Luminanz 70x120s

RGB 3x12x120s

total exposure time: 192 min

20.03.2018

 

Processing: PixInsight

 

I took this during a rare period of consecutive clear nights and was imaged after finishing off the Christmas Tree nebula. This was taken over 2 nights. The conditions were clear but the rather unstable atmosphere made guiding difficult. Though the galaxies are fine I’m not happy with the stars.

 

OBJECT DESCRIPTIONS:-

M65, M 66 & NGC3628 are part off the Leo Triplet. These Galaxies Lie approximately between 31 & 35 million ly from earth.

 

M65 is believed to have very little star formation going on and the number of old stars compered to new ones is quit high. It has a visual magnitude of 10.25.

 

M66 is believed to have had a interaction with NGC3628 in the past resulting in a very high central mass. There have been 5 supernovae observed between 1973 & 2018. It has a visual magnitude of 8.9.

 

NGC3628 also known as the Hamburger Galaxy. it is a unbarred spiral galaxy with a visual magnitude of 10.2.

 

EQUIPMENT:-

Explore Scientific 102mm F7 APO Carbon

Focal Reducer: Explore Scientific 0.7

Mount: AZ-EQ6 GT

ZWO ASI1600mm-Cool cmos camera

Orion Mini Auto Guide

ZWO L,R,G,B Filters

Chip Temp Cooled to -15 degC

 

IMAGING DETAILS:-

M66, M65 and NGC3628 (Leo)

Gain 139 (Unit Gain)

25 Red subs@180sec (1h 15min)

25 Green subs@180sec (1h 15min)

25 Blue subs@180sec (1h 15min)

50 lum subs@120sec (1h 40min)

Total imaging Time 5h 25min

Dithering

20 Darks

20 Flats

 

PROCESSING/GUIDING SOFTWARE:-

N.I.N.A

PHD2

DSS

GraXpert AI

StarNet++

Siril

Affinity photo 2

Situé à environ 35 millions d’années-lumière dans la constellation du Lion, le Triplet du Lion est un petit ensemble de galaxies en interaction gravitationnelle. Il est composé de trois galaxies spirales : M65, M66 et NGC 3628.

M65 et M66 (en bas de l’image) présentent des structures spirales relativement classiques, tandis que NGC 3628 se distingue par une vue par la tranche, marquée par une large bande de poussière sombre qui traverse son disque.

Cependant, cet aspect esthétique masque une histoire dynamique et agitée. Ces galaxies ne sont pas isolées : leurs formes actuelles portent les traces d’interactions gravitationnelles passées. En particulier, M66 et NGC 3628 se seraient rapprochées il y a environ 800 millions d’années, perturbant profondément leur structure interne. Ces interactions ont entraîné des redistributions de gaz et probablement déclenché des épisodes intenses de formation d’étoiles.

Il en résulte une longue traînée qui s’échappe de NGC 3628. S’étendant sur près de 300 000 années-lumière vers le haut et la gauche de l’image. Elle s’est formée lorsque les forces de marée ont arraché de la matière à la galaxie.

Exif :

• 110 poses de 300 secondes (envrion 10h)

• Télescope 200/1000 sur monture NEQ6 Pro GoTo

• Caméra ASI2600MC Pro avec filtre Optolong L-Quad

• Prise de vue en campagne lilloise (ciel Bortle 6)

• Traitement Siril - Pix - Ps

 

-------

 

Located about 35 million light-years away in the constellation Leo, the Leo Triplet is a small group of galaxies in gravitational interaction. It is composed of three spiral galaxies: M65, M66, and NGC 3628.

 

M65 and M66 (at the bottom of the image) display relatively classic spiral structures, while NGC 3628 stands out due to its edge-on view, marked by a wide dark dust lane crossing its disk.

 

However, this striking appearance masks a dynamic and turbulent history. These galaxies are not isolated: their current shapes bear the traces of past gravitational interactions. In particular, M66 and NGC 3628 are believed to have come close about 800 million years ago, deeply disturbing their internal structures. These interactions led to the redistribution of gas and likely triggered intense episodes of star formation.

 

As a result, a long tidal tail extends from NGC 3628, stretching nearly 300,000 light-years toward the upper left of the image. It formed when tidal forces pulled material away from the galaxy.

 

Exif :

• 110 exposures of 300 seconds (about 10 hours)

• 200/1000 telescope on an NEQ6 Pro GoTo mount

• ASI2600MC Pro camera with Optolong L-Quad filter

• Captured from the Lille countryside (Bortle 6 sky)

• Processing: Siril – PixInsight – Photoshop

 

The Leo Triplet is a small group of galaxies in the constellation Leo and include Messier 65 (M65), Messier 66 (M66) and NGC 3628 (a beautiful edge-on spiral galaxy). The trio is estimated to be some 30-million light-years away. In this image, M65 is in the upper right, M66 in the lower right and NGC 3628 on the left.

 

Tech Specs: Sky Watcher Esprit 120ED, ZWO ASI071mc-Pro running at 0C, Celestron CGEM-DX Mount Pier Mounted, ZWO EAF, 121 x 60 second exposures with dark/flat frames, guided using a ZWO ASI290MC and Orion 60mm guide scope, controlled with a ZWO ASIAir Pro. Image date: May 13, 2021. Location: The Dark Side Observatory, Weatherly, PA, USA (Bortle 4 Zone).

A first attempt at the well-known triangle of galaxies known as the Leo Triplet.

On the top, NGC3628 aka the Hamburger galaxy; below, M66 and M65.

 

I'm particularly pleased to have got 3 extra bonus galaxies in the frame: right up in the top-left the tiny fuzzy IC2782, with IC2776 just below and IC2763 in the middle of the left edge of the frame.

 

Nearly two hours' data, Altair 26C at gain 100 with Neodymium filter, 3-minute subs, and plenty darks+flats+bias calibrations as well.

1100mm/F7.3 telescope

Pentax 645z (astro-modified)

total exposure time = 21.5 hr

 

see www.astrobin.com/jjamtq/E/?nc=all for more technical details.

Le triplet du Lion (aussi appelé le groupe de M66) est un petit groupe de galaxies situé à environ 35 millions d'années-lumière dans la constellation du Lion. Cet amas regroupe les galaxies spirales M65, M66, et NGC 3628 , communément appelée "la galaxie du Hamburger".

www.astrobin.com/qtb524/

 

NGC 3628, also known as the Hamburger Galaxy or Sarah's Galaxy, is an unbarred spiral galaxy about 35 million light-years away in the constellation Leo. It was discovered by William Herschel in 1784. It has an approximately 300,000 light-years long tidal tail.

 

Close to 20 hours of integration in LRGB with additional Ha in red channel.

 

Technical card

Imaging telescope or lens:Altair Astro RC250-TT 10" RC Truss Tube

 

Imaging camera:ZWO ASI1600MM-Cool

 

Mount:Mesu 200 Mk2

 

Guiding telescope or lens:Celestron OAG Deluxe

 

Guiding camera:QHYCCD QHY5III174

 

Focal reducer:Riccardi Reducer/Flattener 0.75x

 

Software:Pleiades Astrophoto PixInsight , Seqence Generator Pro

 

Filters:Astrodon R Gen.2 E-series 36mm, Astrodon G Gen.2 E-series 36mm, Astrodon B Gen.2 E-series 36mm, Astrodon HA 36mm - 5nm, Astrodon L Gen.2 E-series 36mm

 

Accessories:TALON6 R.O.R, ZWO EFW, MoonLite NiteCrawler WR30

 

Resolution: 1748x1632

 

Dates:Feb. 2, 2020, Feb. 12, 2020, Feb. 19, 2020, Feb. 21, 2020, Feb. 25, 2020

 

Frames:

Astrodon B Gen.2 E-series 36mm: 45x180" (gain: 75.00) -20C bin 1x1

Astrodon G Gen.2 E-series 36mm: 45x180" (gain: 75.00) -20C bin 1x1

Astrodon HA 36mm - 5nm: 12x600" (gain: 200.00) -20C bin 1x1

Astrodon L Gen.2 E-series 36mm: 220x180" (gain: 75.00) -20C bin 1x1

Astrodon R Gen.2 E-series 36mm: 45x180" (gain: 75.00) -20C bin 1x1

 

Integration: 19.8 hours

 

Avg. Moon age: 16.22 days

 

Avg. Moon phase: 32.64%

 

Astrometry.net job: 3323467

 

RA center: 11h 20' 16"

 

DEC center: +13° 35' 20"

 

Pixel scale: 1.007 arcsec/pixel

 

Orientation: 359.311 degrees

 

Field radius: 0.335

 

Locations: AAS Montsec, Àger, Lleida, Spain

 

Data source: Own remote observatory

 

Remote source: Non-commercial independent facility

Equipment:

GSO RC8 + CCDT67 Reducer

1100mm f5,5

Moravian CCD G2-8300FW10

Astrodon LRGB Filter

Losmandy G11 LFE Photo

 

Guiding:

Starlight Lodestar an Celestron OAG + PHD

 

Date: April 2013

NGC3628 è una galassia a spirale facente parte del famoso tripletto del Leone nella costellazione che porta lo stesso nome. Le sue compagne ben più visibili sono la m65 e m66.

 

E' stata scoperta da William Herschel nel lontano 1784 e la sua caratteristica più evidente è la notevole fascia oscura causata dalla polvere disposta lungo la parte esterna della spirale.

 

La galassia ha una distanza stimata di circa 38 milioni di anni luce basandosi sul redshift z del catalogo NED di 0.002812.

 

Fotografia scattata con l'osservatorio personale 3zObservatory insieme all'amico Giorgio Mazzacurati nel periodo che va dagli ultimi giorni di marzo ai primi di giugno 2019 con una lunga pausa a causa del maltempo. Composizione LRGB circa 10 ore di integrazione a bin2

 

Strumentazione:

 

RC12GSO su EQ8

CCD G24000-Baader Filter LRGB

39x600s L

15x600s per R, 15x600 per G e 15x600 per il B

Elaborazione tramite Pixinsight/Photoshop

Picture saved wThe Leo Triplet is a small group of galaxies in the constellation Leo and include Messier 65 (M65), Messier 66 (M66) and NGC 3628 (a beautiful edge-on spiral galaxy). The trio is estimated to be some 30-million light-years away. In this image, M65 is in the upper right, M66 in the lower right and NGC 3628 on the left.

 

Tech Specs: Sky Watcher Esprit 120ED, Sky-Watcher EQ6R-Pro mount, ZWO ASI2600MC-P camera, 93 x 60 seconds at -10C with darks from the library and flats taken the next morning, guided using a ZWO 30mm f/4 mini guide scope and ZWO 120 Mini, focus using a ZWO EAF. Captured using ZWO AAP and processed using PixInsight. Image date: March 3, 2022. Location: The Dark Side Observatory, Weatherly, PA, USA (Bortle Class 4).ith settings embedded.

Taken w/ Skywatcher Evostar 80ED (w/.85X reducer), Nikon D3300, 100x30s Lights, ~100 bias, ~100 flats, 1600 ISO. Stacked in DeepSkyStacker and Post-processed in Photoshop.

 

This is a re-process of a very old set of data using some new post-processing software.

The Hamburger Galaxy, not my best image as it's quite low in the northern sky from my location and I was exposing while shooting over house roofs which, no doubt, caused thermal currents and destabilised the star and object light.

 

NGC 3628 is a unbarred spiral galaxy, located about 35 million light-years away in the constellation Leo.

Along with M65 and M66, NGC 3628 forms the Leo Triplet, a small group of galaxies. Its most conspicuous feature is the broad and obscuring band of dust located along the outer edge of its spiral arms, roughly resembling meat between bread rolls and giving it the nickname "The Hamburger Galaxy".

 

This image was exposed across two nights, 3 & 4 April 2022, using a QHY268M through a Celestron C8" SCT at the native 2032mm focal length, tracked on a Hypertuned CGEM mount.

 

Total exposure time was 6 hours and 23 minutes through all LRGB filters.

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