Movatterモバイル変換

[0]ホーム
URL:

Jump to content
WikipediaThe Free Encyclopedia
Search

NGC 4605

From Wikipedia, the free encyclopedia
Galaxy in the constellation Ursa Major
NGC 4605
NGC 4605 byHubble.[1]
Observation data (J2000epoch)
ConstellationUrsa Major
Right ascension12h 39m 59.381s[2]
Declination+61° 36′ 33.09″[2]
Redshift0.000484±0.000020[3]
Heliocentric radial velocity143 ± 5km/s[4]
Distance18.10 ± 0.33 Mly (5.55 ± 0.10 Mpc)[5]
Apparent magnitude (V)10.9[4]
Absolute magnitude (B)–18.10[6]
Characteristics
TypeSBc[6] or SB(s)c pec[4]
Mass/Light ratio0.25±0.03[6] M☉/L☉
Apparent size (V)6.03′ × 2.45′[7]
Other designations
UGC 7831,[8]PGC 42408[4]

NGC 4605 is a dwarfbarred spiral galaxy[6] in theconstellationUrsa Major, located at a distance of 18.1 ± 0.3megalight-years from theMilky Way.[5] Physically it is similar in size and inB-band absolute magnitude to theLarge Magellanic Cloud.[6] It is a possible member of either theM81 Galaxy Group or theMessier 101 Group.[9]

References

[edit]
  1. ^"The scale of the Universe".ESA/Hubble Picture of the Week. Retrieved10 May 2014.
  2. ^abSkrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006)."The Two Micron All Sky Survey (2MASS)".The Astronomical Journal.131 (2):1163–1183.Bibcode:2006AJ....131.1163S.doi:10.1086/498708.ISSN 0004-6256.S2CID 18913331.
  3. ^Paturel, G.; et al. (2002). "Comparison LEDA/SIMBAD octobre 2002. Catalogue to be published in 2003".LEDA.Bibcode:2002LEDA.........0P.
  4. ^abcd"NASA/IPAC Extragalactic Database".Results for NGC 4605. Retrieved2010-05-14.
  5. ^abTully, R. Brent; et al. (October 2013). "Cosmicflows-2: The Data".The Astronomical Journal.146 (4): 25.arXiv:1307.7213.Bibcode:2013AJ....146...86T.doi:10.1088/0004-6256/146/4/86.S2CID 118494842. 86.
  6. ^abcdeBolatto, A. D.; et al. (August 2002). "The Density Profile of the Dark Matter Halo of NGC 4605".Astrophysical Journal.565 (1):238–243.arXiv:astro-ph/0108050.Bibcode:2002ApJ...565..238B.doi:10.1086/324596.S2CID 9316982.
  7. ^Paturel, G.; et al. (December 2003)."HYPERLEDA. I. Identification and designation of galaxies".Astronomy and Astrophysics.412:45–55.Bibcode:2003A&A...412...45P.doi:10.1051/0004-6361:20031411.
  8. ^"NGC 4605".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-04-29.
  9. ^Karachentsev, Igor D.; Kaisin, Serafim S. (May 2007). "A View of the M81 Galaxy Group via the Hα Window".The Astronomical Journal.133 (5):1883–1902.arXiv:astro-ph/0701465.Bibcode:2007AJ....133.1883K.doi:10.1086/512127.S2CID 117916931.

External links

[edit]
4001 to 4100
4101 to 4200
4201 to 4300
4301 to 4400
4401 to 4500
4501 to 4600
4601 to 4700
4701 to 4800
4801 to 4900
4901 to 5000


Stub icon

Thisspiral galaxy article is astub. You can help Wikipedia byexpanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=NGC_4605&oldid=1278192469"
Categories:
Hidden categories:
[8]ページ先頭
©2009-2025 Movatter.jp