NGC 7619 + NGC 7626 - Pegasus I Cluster |
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Object data of Pegasus I Cluster |
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Object type: | Galaxy group | |
Size: | 60' | |
Magnitude: | 11.1mag - NGC 7619 / 11.2mag - NGC 7626 | |
Constellation: | Peg | |
Distance: | 150 Mio Ly | |
Notes: |
NGC 7619 and NGC 7626 are the two dominant elliptical galaxy members of the
Pegasus I galaxy group. The Pegasus I cluster contains perhaps 13 galaxies
at a distance of 150 Mio light-years.
This galaxy group is embedded in clouds of galactic cirrus. These clouds, which are better visible in the stretched luminance image, are part of our own Milky Way and hang only hundreds of light-years above our galactic plane, dimly reflecting starlight. |
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Exposure data |
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Date: | 2017-07-19 + 20 + 22 + 23 + 24 (Calima) | |
Location: | ATHOS Centro Astronomico / La Palma (900m) | |
Telescope: | Astro-Physics 175mm f/8 Starfire EDF with field flattener (f=1452mm) | |
Camera: | Moravian G4-16000 with Baader filters | |
Binning: | L 1x1 / RGB 1x1 | |
Mount: | 10micron GM3000 HPS | |
Exposure time: | L 36x6min / R 12x6min / G 12x6min / B 12x6min | |
Exposure time total: | 7h 12min | |
Notes: | Image acquisition by CEDIC team (Bernhard Hubl, Christoph Kaltseis, Markus Blauensteiner, Michael Hanl) Image processing by Bernhard Hubl |
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