Comahopen
| Comahopen | |
|---|---|
 | |
| Observationsdata | |
| Stjärnbild | Berenikes hår |
| Rektascension | 12t 59m 48.7s[1] |
| Deklination | +27° 58′ 50″[1] |
| Avstånd | 350 miljoner[2] l |
| Hopens diameter | 16 miljoner[2] ' |
| Andra beteckningar | |
| ABELL 1656, UGCl 276, CID 90, CAN 090, USGC U508, ZwCl 1257.1+2806, SCL 117 NED02, RASSCALS NRGb 226, PLCKESZ G057.33+88.01, IGR J12595+2755, MAXI J1259+279, 2PBC J1259.5+2756, SAXWFC J1259.5+2756.6, EXSS 1257.4+2815, 1ES 1257+282, XSS J12596+2759, SWIFT J1259.4+2757, SWIFT J1259.7+2755, [ZGH93] G074, [RPG97] 226, [KVC2005] 08, [KRL2007] 128[1] | |
| Se också: Galaxhop Lista över galaxhopar | |
Comahopen är en galaxhop som täcker stora delar av Berenikes hår.[2]
Referenser
Media som används på denna webbplats
Ssc2007-10a1.jpg
This false-color mosaic of the central region of the Coma cluster combines infrared and visible-light images to reveal thousands of faint objects (green). Follow-up observations showed that many of these objects, which appear here as faint green smudges, are dwarf galaxies belonging to the cluster. Two large elliptical galaxies, NGC 4889 and NGC 4874, dominate the cluster's center. The mosaic combines visible-light data from the Sloan Digital Sky Survey (color coded blue) with long- and short-wavelength infrared views (red and green, respectively) from NASA's Spitzer Space Telescope.
This false-color mosaic of the central region of the Coma cluster combines infrared and visible-light images to reveal thousands of faint objects (green). Follow-up observations showed that many of these objects, which appear here as faint green smudges, are dwarf galaxies belonging to the cluster. Two large elliptical galaxies, NGC 4889 and NGC 4874, dominate the cluster's center. The mosaic combines visible-light data from the Sloan Digital Sky Survey (color coded blue) with long- and short-wavelength infrared views (red and green, respectively) from NASA's Spitzer Space Telescope.