IC 423
IC 423 ist ein Emissionsnebel im Sternbild Orion am Himmelsäquator. Das Objekt wurde am 27. Juni 1888 von der US-amerikanischen Astronomin Williamina Fleming e…
| Emissionsnebel | ||
|---|---|---|
| IC 423 | ||
 | ||
| SDSS-Aufnahme | ||
  | ||
| AladinLite | ||
| Sternbild | Orion | |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | ||
| Rektaszension | 05h 33m 22,0s [1] | |
| Deklination | −00° 36′ 52″ [1] | |
| Erscheinungsbild | ||
| Winkelausdehnung | 5,5' × 3,5'[2] | |
| Ionisierende Quelle | ||
| Bezeichnung | IRAS 05307-0038 | |
| Typ | T Tauri Star | |
| Physikalische Daten | ||
| Entfernung | 1056 Lj | |
| Geschichte | ||
| Entdeckung | Williamina Fleming | |
| Datum der Entdeckung | 27. Juni 1888 | |
| Katalogbezeichnungen | ||
| IC 423 • LBN 913 • CB 31 | ||
IC 423 ist ein Emissionsnebel im Sternbild Orion am Himmelsäquator. Das Objekt wurde am 27. Juni 1888 von der US-amerikanischen Astronomin Williamina Fleming entdeckt.[3]
Literatur
- König, Michael & Binnewies, Stefan (2023): Bildatlas der Sternhaufen & Nebel, Stuttgart: Kosmos, S. 52
Weblinks
Einzelnachweise
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