NGC 2032
| Emissionsnebel | ||
|---|---|---|
| NGC 2032 | ||
 | ||
| Aufnahme des Emissionsnebels mit den hervortretenden Komponenten NGC 2029 (unten), NGC 2032 (rechts) und NGC 2035 mithilfe des Very Large Telescope | ||
  | ||
| AladinLite | ||
| Sternbild | Schwertfisch | |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | ||
| Rektaszension | 05h 35m 20,6s [1] | |
| Deklination | −67° 34′ 06″ [1] | |
| Erscheinungsbild | ||
| Ionisierende Quelle | ||
| Physikalische Daten
| ||
| Zugehörigkeit | Große Magellansche Wolke | |
| Geschichte | ||
| Entdeckung | John Herschel | |
| Datum der Entdeckung | 2. November 1834 | |
| Katalogbezeichnungen | ||
| NGC 2032 • GC 1235 • h 2913 • ESO 56-EN160 | ||
NGC 2032 ist ein Emissionsnebel in der Großen Magellanschen Wolke im Sternbild Dorado. Das Objekt wurde am 2. November 1834 von dem Astronomen John Herschel entdeckt.[2]
NGC 2032 gehört zu N59A, einem H-II-Gebiet in der großen Magellanschen Wolke am südöstlichen Rand der Superblase LMC4.
Einzelnachweise
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