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NGC 3156

Today we are going to talk about NGC 3156, a topic that has captured the attention of many in recent times. NGC 3156 is a topic that has generated a lot of controversy and debate in today's society, since it has a great impact on our lives. With the rise of technology and globalization, NGC 3156 has become a relevant topic in all areas, from politics to pop culture. In this article, we will explore the different aspects of NGC 3156 and its influence on our society, and how it is shaping the world we live in.

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NGC 3156
NGC 3156 by Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationSextans
Right ascension10h 12m 41.24591s[1]
Declination+03° 07′ 45.6939″[1]
Redshift0.00415[2]
Heliocentric radial velocity1242 km/s[2]
Distance72.67 ± 0.46 Mly (22.28 ± 0.14 Mpc)[3]
Apparent magnitude (V)12.30[4]
Apparent magnitude (B)13.07[4]
Characteristics
TypeS0[4]
Other designations
UGC 5503, MCG +01-26-019, PGC 29730[2]

NGC 3156 is a lenticular galaxy located in the constellation Sextans.[5][6][7] It is located at a distance of about 75 million light-years from Earth and is forming a pair with NGC 3169. It was discovered by astronomer William Herschel on December 13, 1784.[8]

It is a member of the NGC 3166 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.[9][10]

  • NGC 3156 (SDSS DR14)
    NGC 3156 (SDSS DR14)

References

  1. ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ a b c "NGC 3156". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-18.
  3. ^ Tully, R. Brent; et al. (2013). "Cosmicflows-2: The Data". The Astronomical Journal. 146 (4): 86. arXiv:1307.7213. Bibcode:2013AJ....146...86T. doi:10.1088/0004-6256/146/4/86. S2CID 118494842.
  4. ^ a b c "Search specification: NGC 3156". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-18.
  5. ^ Stone, Nicholas C.; van Velzen, Sjoert (2016-06-30). "An enhanced rate of tidal disruptions in the centrally overdense E+A galaxy NGC 3156". The Astrophysical Journal. 825 (1): L14. arXiv:1604.02056. Bibcode:2016ApJ...825L..14S. doi:10.3847/2041-8205/825/1/L14. S2CID 118479040.
  6. ^ "Central regions of the early-type galaxies in the NGC 3169 group". ResearchGate. Retrieved 2020-09-27.
  7. ^ "A Preferred Home for Disrupted Stars". aasnova.org. American Astronomical Society. 13 July 2016. Retrieved 2020-09-27.
  8. ^ Seligman, Courtney. "New General Catalogue objects: NGC 3150 - 3199". cseligman.com. Retrieved 2021-02-18.
  9. ^ "The Leo III Groups". Atlas of the Universe. Archived from the original on July 22, 2012. Retrieved 2010-11-27.
  10. ^ "NAME NGC 3166 Group". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-18.
  • Media related to NGC 3156 at Wikimedia Commons


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