Field galaxy

A field galaxy is a galaxy that does not belong to a larger galaxy group or cluster and hence is gravitationally alone.

Roughly 80% of all galaxies located within 5 Mpc (16 Mly) of the Milky Way are in groups or clusters of galaxies.[1] Most low-surface-brightness galaxies are field galaxies.[2] The median Hubble-type of field galaxies is Sb, a type of spiral galaxy.[3]

List of field galaxies

A list of nearby relatively bright field galaxies within the Local Volume, about 10 Mpc (33 Mly)[4]

Galaxy Type Size Constellation RA DEC Distance Notes
NGC 404 SA(s)0 Andromeda 01h 09m 27.0s +35° 43 04 11.2 Mly (3.4 Mpc) [4]
NGC 1313 SB(s)d Reticulum 03h 18m 15.4s −66° 29 50 12.89 Mly (3.95 Mpc) Nicknamed the "Topsy Turvy Galaxy" due to its uneven shape [4]
NGC 2188 Sm Columba 06h 10m 09.7s −34° 06 50 27.5 Mly (8.4 Mpc) [4]
NGC 2683 Sc Lynx 08h 52m 41.3s +33° 25 18 32.9 Mly (10.1 Mpc) [4]
NGC 2903 SBbc Leo 09h 32m 10.1s +21° 30 03 30.6 Mly (9.4 Mpc) [4]
NGC 3115 S0 Sextans 10h 05m 14.0s −7° 43 07 31.6 Mly (9.7 Mpc) [4]
NGC 3621 SA(s)d Hydra 11h 18m 16.5s –32° 48 51 21.7 Mly (6.7 Mpc) [4]
NGC 4136 SABc Coma Berenices 12h 09m 17.7s +29° 55 39 40.9 Mly (12.5 Mpc) [4]
NGC 4605 SB(s)c Ursa Major 12h 39m 59.4s +61° 36 33 15.3 Mly (4.7 Mpc) [4]
NGC 5068 SAB(rs)cd Virgo 13h 18m 54.8s −21° 02 21 19.8 Mly (6.1 Mpc) [4]
NGC 6503 SA(s)cd
LINER
30 kly (9.2 kpc) Draco 17h 49m 26.514s +70° 08 39.63 18.5 Mly (5.7 Mpc) Also called the "Lost-In-Space galaxy" due to its location next to the Local Void. [4][5][6][7]

Further reading

  • Piero Madau; Lucia Pozzetti; Mark Dickinson (1998). "The Star Formation History of Field Galaxies". The Astrophysical Journal (published May 1998). 498 (1): 106–116. arXiv:astro-ph/9708220. Bibcode:1998ApJ...498..106M. doi:10.1086/305523.[8]
  • David R. Silva; Gregory D. Bothun (July 1998). "The Ages of Disturbed Field Elliptical Galaxies. I. Global Properties". The Astronomical Journal. 116 (1): 85. Bibcode:1998AJ....116...85S. doi:10.1086/300394.
  • David R. Silva; Gregory D. Bothun (December 1998). "The Ages of Disturbed Field Elliptical Galaxies. II. Central Properties". The Astronomical Journal. 116 (6): 2793. Bibcode:1998AJ....116.2793S. doi:10.1086/300642.
  • Pieter G. van Dokkum (27 June 2005). "The Recent and Continuing Assembly of Field Ellipticals by Red Mergers". The Astronomical Journal (published December 2005). 130 (6): 2647–2665. arXiv:astro-ph/0506661. Bibcode:2005AJ....130.2647V. doi:10.1086/497593.[3]
  • Anatoly Klypin; Igor Karachentsev; Dmitry Makarov; Olga Nasonova (18 May 2014). "Abundance of Field Galaxies". Monthly Notices of the Royal Astronomical Society. 454 (2): 1798–1810. arXiv:1405.4523. Bibcode:2015MNRAS.454.1798K. doi:10.1093/mnras/stv2040.

References

  1. Astronomische Nachrichten, "On the Emptiness of Voids", K.-H. Schmidt; Petra Böhm; Hans Elsässer; vol. 318, no. 2, p. 81, Bibcode:1997AN....318...81S
  2. "An Introduction to Galaxies and Cosmology", David J. Adams and others
  3. Pieter G. van Dokkum (27 June 2005). "The Recent and Continuing Assembly of Field Ellipticals by Red Mergers". The Astronomical Journal (published December 2005). 130 (6): 2647–2665. arXiv:astro-ph/0506661. Bibcode:2005AJ....130.2647V. doi:10.1086/497593.
  4. Jürgen Materne (April 1979). "The structure of nearby groups of galaxies – Quantitative membership probabilities". Astronomy & Astrophysics. 74 (2): 235–243. Bibcode:1979A&A....74..235M.
  5. "Lonely galaxy lost in space". Space Daily. 11 June 2015.
  6. "NGC 6503". NASA/IPAC Extragalactic Database.
  7. "NGC 6503". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 26 February 2018.
  8. Piero Madau; Lucia Pozzetti; Mark Dickinson (1998). "The Star Formation History of Field Galaxies". The Astrophysical Journal (published May 1998). 498 (1): 106–116. arXiv:astro-ph/9708220. Bibcode:1998ApJ...498..106M. doi:10.1086/305523.
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