NGC 341
The NGC 341 topic has been the subject of debate and controversy throughout history. From its origins to the present day, NGC 341 has played a vital role in various aspects of society. In this article, we will explore different facets and perspectives on NGC 341, analyzing its impact on culture, politics, economics and other areas. Additionally, we will examine current trends related to NGC 341 and its influence on the contemporary world. Through an exhaustive analysis, we aim to shed light on the importance and relevance of NGC 341 in the current context, providing a comprehensive and updated vision on this very relevant topic.
| NGC 341 | |
|---|---|
 SDSS image of NGC 341 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 00m 45.8s |
| Declination | −09° 11′ 09″ |
| Redshift | 0.015187 |
| Heliocentric radial velocity | 4,553 km/s< |
| Apparent magnitude (V) | 13.7g |
| Characteristics | |
| Type | SAB(r)bc |
| Apparent size (V) | 1.21' × 1.00' |
| Other designations | |
NGC 341 is a spiral galaxy in the constellation Cetus. It was discovered on October 21, 1881 by Édouard Stephan. It was described by Dreyer as "faint, pretty large, round, a little brighter middle, mottled but not resolved." It has a companion galaxy, PGC 3627, which is sometimes called NGC 341B.[3] For this, reason, it has been included in Halton Arp's Atlas of Peculiar Galaxies.[4]
References
- ^ "NASA/IPAC Extragalactic Database". Results for NGC 0341. Retrieved September 2, 2016.
- ^ "Reference Catalog of galaxy SEDs". Multi-wavelength data on NGC 0341. Retrieved September 16, 2017.
- ^ "New General Catalog Objects: NGC 300 - 349". Cseligman. Retrieved November 4, 2016.
- ^ Arp, Halton (1966). ATLAS OF PECULIAR GALAXIES. Pasadena, California: California Institute of Technology. Retrieved January 5, 2010. (webpage includes PDF link)
External links
Media related to NGC 341 at Wikimedia Commons
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