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NGC 7771,7771A,7770,7769 (Pegasus) * August-September 2017 * ASA N12 astrograph (f/3.6, 1075mm) * ASA DDM85 mount * G3-16200 EC Moravian CCD* LRGB Baader filters * Subframes acquired unguided: Auotslew+ Sequence programms * L: 720 min R: 480min G::420 min B:540 min *
( Thanks to Mr. Sakib Rasool for the image suggestion).
The galactic group of NGC 7771 is about 200 million light-years away in the constellation of Pegasus: NGC 7771 is the large, pebble spiral galaxy of 75,000 light-years in diameter that appears in the center of the image, which is accompanied by two small galaxies beneath it... a lenticular (NGC 7770) and a very small one in it´s border (NGC 7771A). The spiral galaxy is NGC 7769, front view. Galaxies in the NGC 7771 group interact with each other and, within a cosmological scale, are predicted to end up fused into an even larger galaxy. The history of these interactions can be described by following the faint currents of stars plucked from galaxies, distorted by the effect of the gravitational tide caused by the above-mentioned close encounters. NGC 7771 has a huge "tails" implying that the galaxies have already passed very close to each other.
It is not easy to get a clear picture of this galactic group, as more detailed images also reveal the presence of dust clouds in the foreground. These faint dust nebulae, located a few hundred light-years away from us and slightly above the galactic plane, reflect the light of the stars in our own galaxy, the Milky Way.
(Image information credits: APOD, Wikipedia, Michael Ryskamp )
Replace your rusty and twisted sub-frame on your 1967-69 Camaro, 1967-69 Firebird, or 1968-74 Nova with a brand new unit from Hotchkis. Hotchkis takes this beautiful sub-frame and pre installs all the key suspension components making this a truly bolt-on package.
Part # sf-500
Hotchkis Sport Suspension
Toll Free: 888-735-6425
23x180; 34x300 and 4x600 second subframes, iso800.
Total exposure approximately 4 hours 48 minutes.
Imaging:
William Optics ZenithStar II 80 ED,
Modified Canon 350D (Baader ACF-2) with Astronomik CLS filter.
Guiding:
Skywatcher Star Travel 120,
Orion SSAG.
All on
Skywatcher HEQ5 Pro
Stacked in DSS, processed in Fitswork and Gimp.
24th, 25th and 27th March 2017
Cambridge, UK
The Car: 1969 Camaro with a Mast LS7 and a T-56 Magnum Transmission
The Project: The Camaro will be receiving our DSE Hydroformed Subframe, QUADRALink™, 4 point DSE Roll Cage, Mini Tub Kit and Subframe Connectors. The car will also be receiving Baer Brakes, a DSE Super Tank 1000 Series, C&R Radiator, DSE SS Headers and a full custom 3” exhaust system.
The Owner: This is Ronnie Buhr’s first project with DSE. He chose Detroit Speed to transform his car into a Pro-Touring Camaro that will ride and handle better than he ever imagined.
www.detroitspeed.com/Projects/ronnie-buhr-1969-camaro/ron...
The Car: 1969 Camaro with a Mast LS7 and a T-56 Magnum Transmission
The Project: The Camaro will be receiving our DSE Hydroformed Subframe, QUADRALink™, 4 point DSE Roll Cage, Mini Tub Kit and Subframe Connectors. The car will also be receiving Baer Brakes, a DSE Super Tank 1000 Series, C&R Radiator, DSE SS Headers and a full custom 3” exhaust system.
The Owner: This is Ronnie Buhr’s first project with DSE. He chose Detroit Speed to transform his car into a Pro-Touring Camaro that will ride and handle better than he ever imagined.
www.detroitspeed.com/Projects/ronnie-buhr-1969-camaro/ron...
The subframe drooping like this looks scarier and messier than it actually is. There is enough slack in the pipes to allow it to drop without causing any upset to pipes or cables.
I disconnected the HC linkage, which, so I understand, is the only other link to the car.
Safety note:- the small bottle jack was not the only thing supporting the car - other blocks, axle stands and detatched wheels are out of view.
r
This image consists of 13 derotated images composited in WinJUPOS. Each of those 13 images are from the best 300 frames of an 800 frame AVI shot with a Celestron 9.25" Edge HD with 3x Barlow and a Point Grey Flea3 color CCD camera. Those AVI files were stacked in AutoStakkert before being processed in PixInsight. The final composite was touched up in GIMP. The time of the subframes spans from 0931.1 UT to 0941.6 UT. WinJUPOS was able to derotate the clouds of Jupiter, but not the motion of Io or its shadow.
Captured 27 April 2022, ~21:30 hrs ET, Springfield, VA, USA. Bortle 8 skies, Celestron 8 inch SCT at f/6.3 (eff. fl 1290mm), Orion Atlas AZ/EQ-G Pro mount. QHY 294M Pro camera @ -10C, bin 2, exposure 4 seconds, gain 3330, stack of 140 subframes, no calibration frames used. Baader Luminance filter.
Clouds: partly cloudy
Seeing: G
Transparency: 4
Moon phase: ~10%
FOV: 29 x 24 arcmin.
Resolution: 0.9 arcsec/pixel.
Orientation: Up is East.
Ap. mag. 8.4
Ap. size 18.6x7.2 arcmin
Type SAB(s)
Appearance: M 106, large bright spiral galaxy, inclined approx. 45° to line of sight, center is bright and thin lens shape, oval bulge is dimmer with texture, large disc has spotty texture with two thin nearly straight arms containing bright knots. Another smaller dim spiral galaxy NGC 4248 is visible at top right.
From Wikipedia:
Messier 106 (also known as NGC 4258) is an intermediate spiral galaxy in the constellation Canes Venatici. It was discovered by Pierre Méchain in 1781.
M106 is at a distance of about 22 to 25 million light-years away from Earth. It contains an active nucleus classified as a Type 2 Seyfert, and the presence of a central supermassive black hole has been demonstrated from radio-wavelength observations of the rotation of a disk of molecular gas orbiting within the inner light-year around the black hole. NGC 4217 is a possible companion galaxy of Messier 106. A Type II supernova was observed in M106 in May 2014.
M106 has a water vapor megamaser (the equivalent of a laser operating in microwave instead of visible light and on a galactic scale) that is seen by the 22-GHz line of ortho-H2O that evidences dense and warm molecular gas. Water masers are useful for observing nuclear accretion disks in active galaxies. The water masers in M106 enabled the first case of a direct measurement of the distance to a galaxy, thereby providing an independent anchor for the cosmic distance ladder. M106 has a slightly warped, thin, almost edge-on Keplerian disc which is on a subparsec scale. It surrounds a central area with mass 4 × 107M⊙.
It is one of the largest and brightest nearby galaxies, similar in size and luminosity to the Andromeda Galaxy. The supermassive black hole at the core has a mass of (3.9±0.1)×107 M☉.
M106 has also played an important role in calibrating the cosmic distance ladder. Before, Cepheid variables from other galaxies could not be used to measure distances since they cover ranges of metallicities different from the Milky Way's. M106 contains Cepheid variables similar to both the metallicities of the Milky Way and other galaxies' Cepheids. By measuring the distance of the Cepheids with metallicities similar to our galaxy, astronomers are able to recalibrate the other Cepheids with different metallicities, a key fundamental step in improving quantification of distances to other galaxies in the universe.
Cassiopeia widefield, a 4 minutes exposure subframe with Leica Apo-macro-Elmarit-R 100mm F2.8 at F2.8 and EOS 5D-AP by IDAS at ISO 800 on Takahashi EM200 temma 2 Jr equatorial mount, autoguided with FSQ-106ED, hiro-design off-axis guider, Imaging Source DMK21AF04 camera, and PHD guiding in Tainai, Niigata, Japan on August 12, 2008.
The Car: 1969 Camaro with a Mast LS7 and a T-56 Magnum Transmission
The Project: The Camaro will be receiving our DSE Hydroformed Subframe, QUADRALink™, 4 point DSE Roll Cage, Mini Tub Kit and Subframe Connectors. The car will also be receiving Baer Brakes, a DSE Super Tank 1000 Series, C&R Radiator, DSE SS Headers and a full custom 3” exhaust system.
The Owner: This is Ronnie Buhr’s first project with DSE. He chose Detroit Speed to transform his car into a Pro-Touring Camaro that will ride and handle better than he ever imagined.
www.detroitspeed.com/Projects/ronnie-buhr-1969-camaro/ron...
The Car: 1969 Camaro with a Mast LS7 and a T-56 Magnum Transmission
The Project: The Camaro will be receiving our DSE Hydroformed Subframe, QUADRALink™, 4 point DSE Roll Cage, Mini Tub Kit and Subframe Connectors. The car will also be receiving Baer Brakes, a DSE Super Tank 1000 Series, C&R Radiator, DSE SS Headers and a full custom 3” exhaust system.
The Owner: This is Ronnie Buhr’s first project with DSE. He chose Detroit Speed to transform his car into a Pro-Touring Camaro that will ride and handle better than he ever imagined.
www.detroitspeed.com/Projects/ronnie-buhr-1969-camaro/ron...
The subframe on 659 had been damaged in Wales from a rear end shunt. It was not worth repairing as it had been patched in the past with a big patch of steel welded on it. I therefore made some enquires for an AN68C sub frame and finally found one. So Graham was sent off to Birmingham to collect it. This frame will be cleaned and fitted to the bus in due course
One of the sub frames, shot from the terrace, pointing up, but towards Zürich... lots of LP. I'm going to have to find dark skies, soon, I do miss the accessibility of the dark near our old home in Vermont, but love it here in Switzerland.
'89 Mugen upsidedown forks
Poletti tuned rear shock
VRP aluminium gas tank
VRP aluminium rear subframe
Tisberger tuning
Messico exhaust
DLR silencer
The Car: 1969 Camaro with a Mast LS7 and a T-56 Magnum Transmission
The Project: The Camaro will be receiving our DSE Hydroformed Subframe, QUADRALink™, 4 point DSE Roll Cage, Mini Tub Kit and Subframe Connectors. The car will also be receiving Baer Brakes, a DSE Super Tank 1000 Series, C&R Radiator, DSE SS Headers and a full custom 3” exhaust system.
The Owner: This is Ronnie Buhr’s first project with DSE. He chose Detroit Speed to transform his car into a Pro-Touring Camaro that will ride and handle better than he ever imagined.
www.detroitspeed.com/Projects/ronnie-buhr-1969-camaro/ron...