NGC 3925

In this article we will explore the fascinating world of NGC 3925, a topic that has piqued the interest of many people over the years. NGC 3925 has been the subject of numerous studies and research, and its relevance has remained over time. From its origins to its impact on today's society, NGC 3925 has left a significant mark on different aspects of daily life. Through this article, we will delve into the different aspects that make NGC 3925 such a relevant and interesting topic, examining its evolution over time and its influence in different areas. Get ready to immerse yourself in the exciting universe of NGC 3925!

NGC 3925
SDSS image of NGC 3925.
Observation data (J2000 epoch)
ConstellationLeo
Right ascension11h 51m 20.9s[1]
Declination21° 53′ 21″[1]
Redshift0.026482[1]
Heliocentric radial velocity7939 km/s[1]
Distance370 Mly (113 Mpc)[1]
Apparent magnitude (V)15.3[1]
Characteristics
TypeSAB0/a[1]
Size~128,000 ly (39.3 kpc) (estimated)[1]
Apparent size (V)0.65 x 0.45[1]
Other designations
PGC 037078, MCG +04-28-071[1]

NGC 3925 is a barred[2] lenticular galaxy[3][2] and a ring galaxy[2] located about 370 million light-years away[3] in the constellation Leo. It was discovered by astronomer Heinrich d'Arrest on February 19, 1863.[4]

NGC 3925 is classified as a "PAS galaxy" because it contains mostly old stars, with no observable star formation activity. NGC 3925 is also a member of the Coma Supercluster.[5]

See also

References

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 3925. Retrieved 2020-05-17.
  2. ^ a b c "HyperLeda -object description". leda.univ-lyon1.fr. Retrieved 2020-05-17.
  3. ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2020-05-17.
  4. ^ "New General Catalog Objects: NGC 3900 - 3949". cseligman.com. Retrieved 2020-05-16.
  5. ^ Gavazzi, Giuseppe; Savorgnan, Giulia; Fumagalli, Mattia (October 2011). "The complete census of optically selected AGNs in the Coma Supercluster: the dependence of AGN activity on the local environment". Astronomy & Astrophysics. 534: A31. arXiv:1107.3702. Bibcode:2011A&A...534A..31G. doi:10.1051/0004-6361/201117461. ISSN 0004-6361.