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NGC 2997

Coordinates:Sky map09h 45m 38.8s, −31° 11′ 28″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Antlia
NGC 2997
NGC 2997
Observation data (J2000epoch)
ConstellationAntlia
Right ascension09h 45m 38.75379s[1]
Declination−31° 11′ 27.3570″[1]
Heliocentric radial velocity1,088±2 km/s[2]
Distance39.8 megalight-years (12.2 Mpc)[3]
Group orclusterNGC 2997 group
Apparent magnitude (V)10.1[2]
Characteristics
TypeSAB(rs)c[4] or Sc(s)I.3[5]
Size120,000ly (36.65kpc) (estimated)[2]
Apparent size (V)8′.9 × 6′.8[2]
Other designations
ESO 434-35, AM 0943-305,NGC 2997[6],UGCA 181,MCG -05-23-012,PGC 27978[2]

NGC 2997 is a face-onunbarred spiral galaxy about 40[3] millionlight-years away in the faint southernconstellation ofAntlia.[3] It was discovered March 4, 1793 by German-born astronomerWilliam Herschel.J. L. E. Dreyer described it as, "a remarkable object, very faint, very large, very gradually then very suddenly bright middle and 4 arcsec nucleus.[7] This is the brightest galaxy of theNGC 2997 group of galaxies, and was featured on the cover of the first edition ofGalactic Dynamics byJames Binney andScott Tremaine.[8]

This is agrand-design galaxy with a symmetrical, two-armed form.[5] Themorphological classification of NGC 2997 is SAB(rs)c,[4] indicating a weakly-barred spiral galaxy (SAB) with an incomplete ring around the bar (rs) and loosely-woundspiral arms (c). It is inclined at an angle of 40° to theline of sight from the Earth, with themajor axis aligned along aposition angle of 110°.[9] The arms host a series of dusty knots that arestar-forming regions being generated through gas compression fromdensity waves.[5] At the core, the arms converge to form a circumnuclear ring with symmetrically-placed hot spots containingsuper star clusters.[4]

A pair ofsupernova events have been detected in the proximity of this galaxy.CCD images taken October 24, 2003 revealed supernova SN 2003jg, positioned11 east and6″ north of the galactic nucleus.[10] This was determined to be aType Ib/c supernova.[11]Supernova SN 2008eh was reported on July 21, 2008, reaching magnitude 15.0. It was positioned123 east and34″ north of the galactic core.[12]

See also

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References

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  1. ^abBrown, 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 atVizieR.
  2. ^abcde"NASA/IPAC Extragalactic Database".Results for NGC 2997. Retrieved2006-11-25.
  3. ^abcHess, K. M.; et al. (2009). "Anomalous HI in NGC 2997".The Astrophysical Journal.699 (1):76–88.arXiv:0904.3494v1.Bibcode:2009ApJ...699...76H.doi:10.1088/0004-637X/699/1/76.S2CID 17931955.
  4. ^abcElmegreen, Debra Meloy; et al. (August 1999)."Near-Infrared Observations of Hot Spots in the Circumnuclear Rings of NGC 2997 and NGC 6951".The Astronomical Journal.118 (2):777–784.Bibcode:1999AJ....118..777E.doi:10.1086/300970.
  5. ^abcGrosbøl, P.; Dottori, H. (June 2009)."Pattern speed of main spiral arms in NGC 2997. Estimate based on very young stellar complexes".Astronomy and Astrophysics.499 (3):L21 –L24.arXiv:0904.4757.Bibcode:2009A&A...499L..21G.doi:10.1051/0004-6361/200911805.hdl:10183/99267.
  6. ^"NGC 2997".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-09-15.
  7. ^Seligman, Courtney."NGC Objects: NGC 2950 - 2999".Celestial Atlas. Retrieved2016-03-01.
  8. ^Binney, J.; Tremaine, S."Galactic Dynamics".Princeton University Press. Archived fromthe original on 2007-04-20. Retrieved2007-04-09.
  9. ^Ho, I. -Ting; et al. (October 2018). "Azimuthal variations of gas-phase oxygen abundance in NGC 2997".Astronomy & Astrophysics.618: 13.arXiv:1807.02043.Bibcode:2018A&A...618A..64H.doi:10.1051/0004-6361/201833262.S2CID 53692123. A64.
  10. ^Martin, R.; Biggs, J. (October 2003). Green, D. W. E. (ed.). "Supernova 2003jg in NGC 2997".IAU Circular.8235: 1.Bibcode:2003IAUC.8235....1M.
  11. ^Kuncarayakti, H.; et al. (May 2018). "Constraints on core-collapse supernova progenitors from explosion site integral field spectroscopy".Astronomy & Astrophysics.613: 18.arXiv:1711.05765.Bibcode:2018A&A...613A..35K.doi:10.1051/0004-6361/201731923.S2CID 55845396. A35.
  12. ^Monard, L. A. G. (July 2008). Green, D. W. E. (ed.). "Supernova 2008eh in NGC 2997".Central Bureau Electronic Telegrams.1445: 1.Bibcode:2008CBET.1445....1M.

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