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NGC 2903

Coordinates:Sky map09h 32m 10.1s, +21° 30′ 03″
From Wikipedia, the free encyclopedia
Spiral galaxy in the constellation Leo
NGC 2903
Anultraviolet image of NGC 2903 taken withGALEX.
Observation data (J2000epoch)
ConstellationLeo
Right ascension09h 32m 10.111s[1]
Declination+21° 30′ 02.99″[1]
Redshift556±1 km/s[2]
Distance30.4 Mly (9.33 Mpc)[3]
Group orclusterVirgo Supercluster[4]
Apparent magnitude (V)9.0[5]
Characteristics
TypeSBbc[6] or SAB(rs)bc[7]
Size100,000 ly (diameter)
Apparent size (V)11.48 × 5.25[8]
Other designations
UGC 5079, IRAS 09293+2143,[9]PGC 27077[2]

NGC 2903 is an isolatedbarred spiral galaxy in theequatorialconstellation ofLeo, positioned about 1.5° due south ofLambda Leonis.[10] It was discovered by German-born astronomerWilliam Herschel, who cataloged it on November 16, 1784. He mistook it as a doublenebula, as did subsequent observers, and it wasn't until the nineteenth century that theThird Earl of Rosse resolved into a spiral form.[5]J. L. E. Dreyer assigned it the identifiers 2903 and 2905 in hisNew General Catalogue; NGC 2905 now designates a luminous knot in the northeasternspiral arm.[11]

Thisfield galaxy[12] is located about 30[3] millionlight-years away from theMilky Way, and is a member of theVirgo Supercluster.[4] Themorphological classification of this galaxy is SBbc,[6] indicating a barred spiral (SB) with moderate to tightly-wound spiral arms (bc).De Vaucouleurs and associates assigned it the class SAB(rs)bc, suggesting a weaker bar structure (SAB) with a partial ring (rs). The bar structure appears stronger in thenear infrared band. The galaxy as a whole is inclined by an angle of 60° to the line of sight from the Earth.[7]

72% of the stellar mass is located in the outer disk of the galaxy, and 20% is found in the bar. The bulge adds 5% of the stellar mass, and its star population is generally older.[13] However, the central~650 pc radius volume of the core is a strongstarburst region. Thestar formation rate here is0.7 M y−1 and it is being fed by gas inflow along the bar. There is no evidence of anactive nucleus.[7]

The irregulardwarf galaxy KKH 51 appears to be a companion, as they have an angular separation of25 and nearly the sameradial velocity.[14]

References

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  1. ^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.
  2. ^ab"NASA/IPAC Extragalactic Database".Results for NGC 2903. Retrieved2006-11-25.
  3. ^abTully, R. Brent; et al. (August 2016)."Cosmicflows-3".The Astronomical Journal.152 (2): 21.arXiv:1605.01765.Bibcode:2016AJ....152...50T.doi:10.3847/0004-6256/152/2/50.S2CID 250737862. 50.
  4. ^ab"Nearby Groups of Galaxies".ned.ipac.caltech.edu. Retrieved2018-05-03.
  5. ^abO'Meara, Stephen James (2007).Hidden treasures. Cambridge University Press. p. 256.ISBN 9780521837040.
  6. ^abAnn, H. B.; et al. (2015). "A Catalog of Visually Classified Galaxies in the Local (z ~ 0.01) Universe".The Astrophysical Journal Supplement Series.217 (2):27–49.arXiv:1502.03545.Bibcode:2015ApJS..217...27A.doi:10.1088/0067-0049/217/2/27.S2CID 119253507.
  7. ^abcYukita, Mihoko; et al. (October 2012). "Hot Diffuse Emission in the Nuclear Starburst Region of NGC 2903".The Astrophysical Journal.758 (2): 17.arXiv:1209.5443.Bibcode:2012ApJ...758..105Y.doi:10.1088/0004-637X/758/2/105.S2CID 119197597. 105.
  8. ^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.
  9. ^"NGC 2903".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-09-14.
  10. ^Sinnott, Roger W.; Perryman, Michael A. C. (1997).Millennium Star Atlas. Vol. 2. Sky Publishing Corporation and the European Space Agency. p. 686.ISBN 0-933346-83-2.
  11. ^Moore, S. L.; et al. (April 2010). "NGC 2903 - the galaxy Messier missed".Journal of the British Astronomical Association.120 (2):106–107.Bibcode:2010JBAA..120..106M.
  12. ^Materne, J. (April 1979). "The structure of nearby groups of galaxies - Quantitative membership probabilities".Astronomy and Astrophysics.74 (2):235–243.Bibcode:1979A&A....74..235M.
  13. ^Carrillo, Andreia; et al. (April 2020)."The VIRUS-P Exploration of Nearby Galaxies (VENGA): the stellar populations and assembly of NGC 2903's bulge, bar, and outer disc".Monthly Notices of the Royal Astronomical Society.493 (3):4094–4106.arXiv:2002.02858.Bibcode:2020MNRAS.493.4094C.doi:10.1093/mnras/staa397.
  14. ^Makarova, L. N.; et al. (March 2002). "Surface photometry of new nearby dwarf galaxies".Astronomy and Astrophysics.384:72–80.arXiv:astro-ph/0201234.Bibcode:2002A&A...384...72M.doi:10.1051/0004-6361:20020006.S2CID 14551920.

External links

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