NGC 1929
| Emissionsnebel | ||
|---|---|---|
| NGC 1929 | ||
 | ||
| Zentrale Region der Nebelstruktur N44, NGC 1929 (o.r) | ||
  | ||
| AladinLite | ||
| Sternbild | Schwertfisch | |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | ||
| Rektaszension | 05h 21m 36,0s [1] | |
| Deklination | −67° 54′ 43″ [1] | |
| Erscheinungsbild | ||
| Ionisierende Quelle | ||
| Physikalische Daten
| ||
| Zugehörigkeit | Große Magellansche Wolke | |
| Geschichte | ||
| Entdeckung | James Dunlop | |
| Datum der Entdeckung | 27. September 1826 | |
| Katalogbezeichnungen | ||
| NGC 1929 • ESO 56-SC107 • GC 1135 • h 2840 • | ||
NGC 1929 ist die Bezeichnung eines Emissionsnebels im Sternbild Dorado.
Das Objekt wurde am 27. September 1826 von dem britischen Astronomen James Dunlop entdeckt.[2]
Literatur
- König, Michael & Binnewies, Stefan (2023): Bildatlas der Sternhaufen & Nebel, Stuttgart: Kosmos, S. 314
Einzelnachweise
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