NGC 1934
In this article, we will explore the fascinating world of NGC 1934 and everything it has to offer. From its origins to its impact on today's society, we will dive into every relevant aspect of NGC 1934, offering a complete and detailed overview. We will analyze its importance in different areas, as well as its role in history and its future relevance. This article is intended to serve as a comprehensive guide to NGC 1934, providing readers with a comprehensive understanding of this fascinating topic.
| Emission nebula | |
|---|---|
 NGC 1934, just above the centre, with NGC 1929 just to the right of the centre and NGC 1937, which is at the far top left | |
| Observation data: epoch | |
| Right ascension | 05h 21m 54.0s[1] |
| Declination | −67° 54′ 54″[1] |
| Apparent magnitude (V) | 10.50 [2] |
| Constellation | Dorado |
| Designations | ESO 56-SC109 |
NGC 1934 (also known as ESO 56-SC109) is an emission nebula located in the Dorado constellation and part of the Large Magellanic Cloud. It was discovered by John Herschel on November 23, 1834.[3] Its apparent magnitude is 10.50.[2]
References
- ^ a b "Object: NGC 1934 (*)". SEDS. Retrieved 14 October 2017.
- ^ a b "NGC 1934 -- Interstellar matter". SIMBAD. Retrieved 14 October 2017.
- ^ "NGC 1934 (in the Large Magellanic Cloud)". cseligman. Retrieved 14 October 2017.
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