IC 2177
| Emissionsnebel | |
|---|---|
| IC 2177 | |
 | |
| Detailaufnahme von IC 2177 durch den Wide Field Imager am MPG/ESO 2,2-Meter-Teleskop. | |
| AladinLite | |
| Sternbild | Einhorn |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 07h 04m 36,9s[1] |
| Deklination | -10° 28′ 16″[1] |
| Erscheinungsbild | |
| Winkelausdehnung | 20'0[2] |
| Ionisierende Quelle | |
| Bezeichnung | HD 53367 (Be star) |
| Physikalische Daten | |
| Entfernung | 3650 Lj (1120 pc) |
| Geschichte | |
| Entdeckung | Isaac Roberts |
| Datum der Entdeckung | 1898 |
| Katalogbezeichnungen | |
| IC 2177 • LBN 1027, vdB 93, Sh2-292 | |
IC 2177 (Seemöwennebel) ist ein Emissionsnebel im Sternbild Einhorn. Das Objekt wurde im Jahre 1898 von Isaac Roberts entdeckt.[3]
Einzelnachweise
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Seagull Nebula.jpg
Autor/Urheber: ESO, Lizenz: CC BY 4.0
This image from ESO’s La Silla Observatory shows part of a stellar nursery nicknamed the Seagull Nebula. This cloud of gas, known as Sh 2-292, RCW 2 and Gum 1, seems to form the head of the seagull and glows brightly due to the energetic radiation from a very hot young star lurking at its heart. The detailed view was produced by the Wide Field Imager on the MPG/ESO 2.2-metre telescope.
Autor/Urheber: ESO, Lizenz: CC BY 4.0
This image from ESO’s La Silla Observatory shows part of a stellar nursery nicknamed the Seagull Nebula. This cloud of gas, known as Sh 2-292, RCW 2 and Gum 1, seems to form the head of the seagull and glows brightly due to the energetic radiation from a very hot young star lurking at its heart. The detailed view was produced by the Wide Field Imager on the MPG/ESO 2.2-metre telescope.