Fujinon GF55mmF1.7 R WR
View allAll Photos Tagged WR
Astro-Physics Riccardi-Honders 305mm @ F/3.65
Moravian C3 61000 + Chroma L, Ha, [O III]
Astro Physics 1200
Astro-Physics 130 GTX + QUADTCC @ F/4.5
Moravian G3 11002 + Astrodon RGB
Astro Physics 1200
Ha: 40x300s bin 1x1
[O III]: 51x300s bin 1x1
RGB: 25x300s bin 1x1
Total exposure: 16h
Captured with Sequence Generator Pro
Processed with Pixinsight
Astro-Physics Riccardi-Honders 305mm @ F/3.65
Moravian C3 61000 + Chroma Ha, [O III], [S II] 8nm
Astro Physics 1200
Ha: 40x300s bin 1x1
[O III]: 51x300s bin 1x1
[S II]: 20x300s bin 1x1
Total exposure: 10h
Captured with Sequence Generator Pro
Processed with Pixinsight
Fujifilm X-T50
XF16-50mmF2.8-4.8 R LM WR
30分に1本の電車を待ってベンチに座っていた。のんびりとこういう時間もいいものだ＾＾
She was sitting on a bench waiting for the train that comes once every 30 minutes. It's nice to have a relaxing time like this.
Doppelt gemoppelt. das Schweriner Schloss einmal etwas anders ...
Eine ungewollte Aufnahme, weil ich vergessen hatte die Kamera umzustellen, nachdem ich vorher eine Mehrfachbelichtung aufgenommen habe.
Terminal Railroad of St. Louis's 101 crew has pulled across the diamonds at WR Tower to deliver a string of empty tank cars for the Port Harbor RR for storage. The train will have to be cut in half due to the length of the lead the TRRA uses to reach the PHRR.
Interested in purchasing a high-quality digital download of this photo, suitable for printing and framing? Let me know and I will add it to my Etsy Shop, MittenRailandMarine! Follow this link to see what images are currently listed for sale: www.etsy.com/shop/MittenRailandMarine
If you are interested in specific locomotives, trains, or freighters, please contact me. I have been photographing trains and ships for over 15 years and have accumulated an extensive library!
WR 134 è una stella di Wolf-Rayet variabile, appartenente alla costellazione del Cigno, distante circa 5 700 al dal Sole, 400.000 volte piu luminosa del sole e terribilmente calda!!
WR 134 perde massa a ritmi esorbitanti, tramite venti stellari molto veloci che danno origine alla debole nebulosa di colore azzurro
Strumentazione:
Telescopio: Newton Vixen R200SS
Camere Di Acquisizione: ZWO ASI2600MC DUO
Montatura: Sky-Watcher EQ6-R Pro
Filtro: Antlia ALP-T Dual Band 5nm 2"
Accessori: ASA 3" 0.95x Wynne Coma Corrector
Software di elaborazione: Pleiades Astrophoto PixInsight · Russell Croman Tools
Riprese del: 09 -10 -11 - 12 Luglio 2024
Fotogrammi:
Antlia ALP-T Dual Band 5nm 2": 60×30,″(30′)
Antlia ALP-T Dual Band 5nm 2": 245×300,″(20h 25′)
Integrazione: 20h 55′
Età lunare media: 4.75 giorni
Fase lunare media: 24.05%
Campionamento: 1,021 arcsec/pixel
Piena risoluzione qui: [astrob.in/mezkb1/0/](astrob.in/mezkb1/0/)
Our young male likes to pose for the camera so I take advantage of his handsomeness whenever he's in the mood.
Fujifilm ACROS simulation with no post processing. SOOC
Pondered what this may look like in Mono ..
Pentax K1 w DFA15-30/2.8
ISO2000 f/4 x 12 frames.
Raw developed in DxO PhotoLab, stacked as raw files in Starry Landscape Stacker, colour graded and IR converted in Color Efex Pro 5, couple of tweaks in Affinity Photo 2, the usual denoise in Topaz and a final stop back in PhotoLab.
Werr Beach, Gerringong, NSW
TECHNICAL DATA:
"FarLightTeam" robotic remote observatory located in “E-EYE Entre Encinas y Estrellas” (Fregenal de la Sierra) Badajoz, Spain.
Team: José Esteban, Jesús M. Vargas, Bittor Zabalegui, Marc Valero
Telescope: Takahashi FSQ106 ED 530mm f/5
Camera: Atik Apx60 ( 9576 x 6388 )
Filters: Astrodom Halpha-OIII
Mount: 10 micron GM1000 HPS
Imaging Software: Voyager
Processing software: PixInsight
IMAGE DATA:
Date: August 2024
47 x 600" Ha
41 x 600" OIII
Total 15 hours of Lights
Calibration shots: Darks, Flats, Bias
Processed by: Jesús M. Vargas
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WR 134 is a Wolf–Rayet variable star located about 6,000 light-years from Earth in the constellation Cygnus , surrounded by a faint bubble nebula driven by the star's intense radiation and fast wind. It is five times the radius of the Sun, but due to a temperature exceeding 63,000 K it is 400,000 times more luminous than the Sun .
WR 134 was one of three stars in Cygnus observed in 1867 that had unusual spectra consisting of intense emission lines rather than the more normal absorption and continuum lines. These were the first members of the class of stars that came to be called Wolf–Rayet stars (WR stars) after their unusual appearance was discovered by Charles Wolf and Georges Rayet. It is a member of the nitrogen sequence of WR stars, while the other two (WR 135 and WR 137) are members of the carbon sequence that also have OB companions. WR 134 has a spectrum with N III and N IV emission between two and five times stronger than NV, leading to the assignment of a WN6 spectral type. The spectrum also shows strong He II emission and weaker He I and C IV lines.
WR 134 is classified as an Algol-type eclipsing variable and has been given the designation V1769 Cygni, but the variation is not strictly periodic and brightness changes occur on timescales of hours to days.
Both hard and soft X-rays have been detected from WR 134, but their origin has not been fully explained. The emissions do not correspond to any star of the expected temperature, they are not sufficient to generate winds that would cause two hot stars to collide, and any compact source, such as a neutron star or a cold dwarf, would be in an unlikely orbit.
I've always thought Wolf-Rayet stars are so cool: ever since Hubble captured the iconic image of WR 124 (seriously look it up if you haven't seen it, it's I've always Wolf-Rayet stars are so cool: ever since Hubble captured the iconic image of WR 124 (seriously look it up if you haven't seen it, it's unreal), I've had this fascination with them. WR 134 is one such star located around 6,000 light years away in the constellation of Cygnus: it's the bright one at the center of the frame. While it is only five times the radius of the sun, but it burns incredibly hot, at over 63,000 K (that's 113,000 degrees Fahrenheit), and is **400,000** times as luminous as the Sun.
This image comprises over 300 five minute exposures from my backyard, or about 28 hours of data, focused on ionized hydrogen and oxygen. What makes the nebula you see here is the incredibly strong solar wind and radiation Wolf-Rayet stars are known for colliding with the surrounding interstellar medium. To give you an idea of the kind of power we are talking about here, this frame is over 50 light years across, and I was fortunate enough to be able to see it from my backyard. Still blows my mind when I think of it.
I continued to work on new Pixinsight techniques in this image. I used Muredenoise for the first time on the linear Oiii master, since it still had a little bit of noise despite the lengthy integration time. I was very pleased with the results: I’ll be building it into the linear workflow from here on out. I also tried Adam Block's star de-emphasis technique where you create a mask with halos around all the stars, cores protected, and replace the halo pixels with median sky pixels from the local area. I love it: I think it gives results superior to simply erosion via MT alone. I had intended to capture some RGB data for the star colors, but I think it turned out ok without it. Plus, I'm eager to move on to the next target. Imaging nights have been few and far between with all the rain we have been having, plus the smoke from the wildfires out west, and I want to make the most of it. Clear skies everyone. Stay safe.
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OOUK CT8, Paracorr II, Moonlite focuser
ASI1600 Pro imaging cam, ASI 290 guide cam
Chroma 5nm Ha: 163 x 300"
Chroma 3nm Oiii: 172 x 300"
Skywatcher EQ6-R Pro
Pegasus Ultimate PowerBox2
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Processing
WBPP script to create masters
Deconvolution using External PSF and a black-clipped mask
DBE on Oiii
MureDenoise script on Oiii
HT to create non-linear Ha and Oiii
HDRMT on both
Pixelmath to combine:
R: iif(ha > .15, ha, (ha*.8)+(oiii*.2))
G: iif(ha > 0.5, 1-(1-oiii)*(1-(ha-0.5)), oiii *(ha+0.5))
B: iif(oiii > .1, oiii, (ha*.3)+(oiii*.2))
Adam Block's star de-emphasis technique (see his website, and my description above).
CurvesTransformation to adjust colors, keeping a star mask in place to protect stars from oversaturation
Imported to Photoshop and Lightroom, then adjusted colors to suit. Also selective, light application of Camera Raw filter with negative adjustments to texture and clarity as a smoothing application.
Oddly enough, I never really did any major denoising aside from MureDenoise at the beginning. I usually use TGVDenoise.
Save for web.