Arp 300
| Galaxie Arp 300 | |
|---|---|
 | |
| Hubble-Weltraumteleskop (Helligkeit) und Pan-STARRS (Farbe) | |
| AladinLite | |
| Sternbild | Großer Bär |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 09h 27m 56,3s[1] |
| Deklination | +68° 24′ 27″ [1] |
| Erscheinungsbild | |
| Morphologischer Typ | DBL SYS [1] |
| Helligkeit (B-Band) | 13,9 mag |
| Physikalische Daten | |
| Rotverschiebung | 0,012008 [1] |
| Radialgeschwindigkeit | 3600 km/s [1] |
| Hubbledistanz vrad / H0 | (165 ± 12) · 106 Lj (50,7 ± 3,6) Mpc [1] |
| Geschichte | |
| Katalogbezeichnungen | |
| UGC 5028/5029 • PGC 26849/26864 • CGCG 332-050/332-051 • MCG +12-09-049/050 • IRAS 09235+6837 • Arp 300 • Mrk 111 • VV 106 • VII Zw 280 | |
Arp 300 ist ein wechselwirkendes Galaxienpaar im Sternbild Großer Bär, das etwa 165 Millionen Lichtjahre von der Milchstraße entfernt ist. Halton Arp gliederte seinen Katalog ungewöhnlicher Galaxien nach rein morphologischen Kriterien in Gruppen. Dieses Galaxienpaar gehört zu der Klasse Unklassifizierte Doppelgalaxien.
Weblinks
Literatur
- Jeff Kanipe und Dennis Webb: The Arp Atlas of Peculiar Galaxies – A Chronicle and Observer´s Guide, Richmond 2006, ISBN 978-0-943396-76-7
Einzelnachweise
Auf dieser Seite verwendete Medien
Autor/Urheber: Judy Schmidt from USA, Lizenz: CC BY 2.0
A spiral galaxy, an edge-on disk, a few other background goodies, and a remarkable pair of dwarf galaxies. The bright pair near the right side of the frame could be an interacting pair, or, interestingly perhaps an overlapping line-of-sight pair, though I really have no way of confirming that. Pay close attention to the reddish/yellowish dust around that bright nucleus at the bottom. See how it encircles the nucleus without looking all that disturbed? Maybe they aren't interacting. Or maybe if they are, it's at an early point. Either way, it's very interesting to see backlit dust in the outskirts of a galaxy. It's usually invisible to us at these wavelengths.
Color comes from PanSTARRS this time.
Establishing HST's Low Redshift Archive of Interacting Systems
Luminosity: ACS/WFC F606W Red: PanSTARRS z Green: PanSTARRS i Blue: PanSTARRS g
North is 24.50° clockwise from up.