NGC 1910
Today, NGC 1910 is a topic of great relevance and interest to people around the world. Since its emergence, NGC 1910 has captured the attention of experts and fans alike, generating constant debate about its importance and impact on different areas of society. In this article, we will thoroughly explore the most relevant aspects of NGC 1910, examining its history, its current implications and its possible evolution in the future. Through comprehensive analysis, we hope to provide our readers with a more complete view of this phenomenon and help them understand its true scope.
| NGC 1910 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Right ascension | 5h 18m 42.5s[1] |
| Declination | −69° 14′ 12.1″[1] |
| Distance | 160,000 ly (50,000 pc) |
| Apparent magnitude (V) | 11.2 [2] |
| Apparent dimensions (V) | 1.54′ (arcmin.)[1] |
| Physical characteristics | |
| Radius | 71.675 (21.975 pc)[note 1] |
| Other designations | NGC 1910, ESO 56-SC99 |
| Associations | |
| Constellation | Dorado |
NGC 1910, or LH-41, is an OB association in the Large Magellanic Cloud.
Location
NGC 1910's right ascension is 5h 18m 42.5s and its declination is -69° 14′ 12.1″.[3] Its angular size is 1.54 arcminutes.[1]
N119
The cluster has an associated HII region called N119.
Stars
NGC 1910 contains several stars including S Doradus, LH41-1042, LMC195-1, and R85.
See also
Notes and references
- ^ Calculated based on size and distance
- ^ a b c d "SIMBAD search results for NGC 1910". Astronomical Database. Retrieved 17 November 2016.
- ^ "Revised NGC Data for NGC 1910". Retrieved 11 December 2016.
- ^ "NED results for object NGC 1910". Retrieved 11 December 2016.
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