NGC 1873
The topic of NGC 1873 is one that always generates great interest and debate among experts and the general public. With a history dating back many years, NGC 1873 has been the subject of numerous studies, research and discussions in various disciplines. From its impact on society to its influence on the economy, NGC 1873 has proven to be a topic of great relevance today. In this article, we will explore the different aspects of NGC 1873, from its origins to its current situation, in order to offer a complete and up-to-date view of this important topic.
| NGC 1873 | |
|---|---|
 NGC 1873, just right of centre, with NGC 1869 below it | |
| Observation data (J2000 epoch) | |
| Right ascension | 05h 13m 55.7s[1] |
| Declination | −67° 20′ 04″[1] |
| Apparent magnitude (V) | 10.4[2] |
| Physical characteristics | |
| Other designations | ESO 85-SC54 |
| Associations | |
| Constellation | Dorado |
NGC 1873 (also known as ESO 85-SC54) is an open cluster associated with an emission nebula located in the Dorado constellation within the Large Magellanic Cloud. It was discovered by James Dunlop on September 24, 1826 and rediscovered by John Herschel on January 2, 1837. Its apparent magnitude is 10.4, and its size is 3.50 arc minutes.[2][3]
NGC 1873 is part of a triple association with NGC 1869 and NGC 1871.[3]
References
- ^ a b "Object: NGC 1873 (*)". spider.seds. Retrieved 14 October 2017.
- ^ a b "NGC 1873". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 14 October 2017.
- ^ a b "NGC 1873 (= an OCL and EN in the LMC)". cseligman. Retrieved 14 October 2017.
