NGC 4308

Today we come across a topic that has sparked growing interest in recent weeks: NGC 4308. This person/topic/date has captured the public's attention and generated intense debate in society. That is why in this article we aim to shed light on the fundamental aspects related to NGC 4308, offering a detailed analysis of its implications and consequences. Along these lines, we will explore the different angles from which NGC 4308 can be approached, with the aim of providing a complete and objective view on this matter. Without a doubt, this is a highly relevant topic that deserves to be addressed with depth and rigor, and that is precisely what we intend to achieve in the following lines.

NGC 4308
A near-infrared image of NGC 4308.
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 21m 56.9s[1]
Declination+30° 04′ 27″[1]
Redshift589 ± 10 km/s[1]
Apparent magnitude (V)14.4[1]
Characteristics
TypeE[1]
Apparent size (V)0.8′ × 0.7′[1]
Other designations
UGC 7426,[1] PGC 40011[1]

NGC 4308 is an elliptical galaxy in the constellation Coma Berenices. It is a member of the Coma I Group.[2]

References

  1. ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 4308. Retrieved 2007-03-30.
  2. ^ Gregory, Stephen A.; Thompson, Laird A. (April 1977). "The Coma i Galaxy Cloud". The Astrophysical Journal. 213: 345–350. Bibcode:1977ApJ...213..345G. doi:10.1086/155160. ISSN 0004-637X.
  • Media related to NGC 4308 at Wikimedia Commons


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