NGC 1929 (also known as ESO 56-EN107) is an open cluster associated with the emission nebula located within the N44 nebula in the Dorado constellation and part of the Large Magellanic Cloud.[3] It was discovered by James Dunlop on August 3, 1826.[4] Its apparent magnitude is 14.0, and its size is 0.8 arc minutes.[2]
| Nebula | |
|---|---|
 NGC 1929, just right of centre, with NGC 1934 just to the left of the centre and NGC 1937, which is at the far top left | |
| Observation data: epoch | |
| Right ascension | 05h 21m 37.0s[1] |
| Declination | −67° 54′ 48″[1] |
| Apparent magnitude (V) | 14.0 [2] |
| Constellation | Dorado |
| Designations | ESO 56-EN107 |
References
edit- ^ a b "Object: NGC 1929 (*)". SEDS. Retrieved 14 October 2017.
- ^ a b "NGC 1929 -- Cluster of Stars". SIMBAD. Retrieved 14 October 2017.
- ^ "NGC 1929 in N44: A Surprisingly Bright Superbubble Space wallpaper". Space.com. 12 September 2012. Retrieved 14 October 2017.
- ^ "NGC 1929 (in the Large Magellanic Cloud)". cseligman. Retrieved 14 October 2017.
External links
edit
Media related to NGC 1929 at Wikimedia Commons
 | This star cluster–related article is a stub. You can help Wikipedia by expanding it. |