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NGC 759

From Wikipedia, the free encyclopedia
Galaxy in the constellation Andromeda
NGC 759
2MASS image of NGC 759.
Observation data (J2000epoch)
ConstellationAndromeda
Right ascension01h 57m 50.3s[1]
Declination36° 20′ 35″[1]
Redshift0.015567[1]
Heliocentric radial velocity4667 km/s[1]
Distance230 Mly (70.4 Mpc)[1]
Group orclusterAbell 262
Apparent magnitude (V)13.3[1]
Characteristics
TypeE[1]
Size~110,000 ly (33 kpc) (estimated)[1]
Apparent size (V)1.6 × 1.4[1]
Other designations
MCG 6-5-67, PGC 7397, UGC 1440[1]

NGC 759 is anelliptical galaxy located 230 millionlight-years away[2] in theconstellationAndromeda. NGC 759 was discovered by astronomer byHeinrich d'Arrest on September 17, 1865.[3] It is a member ofAbell 262.[4][5][6][7][8]

Despite being classified as aradio galaxy,[9][10][11][12][13] the radio emission in NGC 759 could be due tostar formation rather than anactive galactic nucleus.[12][13]

Dust disk

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The central region of NGC 759 harbors a face-on dust disk with tightly wound spiral structure. The disk has a diameter of 11,000 ly (3.4 kpc).[14] The dust disk also contains a smaller circumnuclear molecular gas ring that has star formation inH II regions.[15][16] These features may be the result of amerger of gas-rich disk galaxies[15][16][17] or by theaccretion of gas-rich material. In either scenario, the gas would have lost momentum and fallen to the center of the galaxy to produce the disk and current star formation.[17] However, Vlasyuk et al. suggests that the disk and the smaller circumnuclear molecular gas ring with star formation inside the main disk formed from a tidal encounter between NGC 759 and a large spiral galaxy which was accompanied by a substantial gas accretion.[16]

The dust disk in NGC 759 as imaged by theHubble Space Telescope

Molecular gas

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NGC 759 contains 2.4 billionM☉ ofmolecular gas. Most of the gas is concentrated in a circumnuclear molecular gas ring with a diameter of 4,200 ly (1.3 kpc).[15] The gas may be the result of the same merger event that produced the circumnuclear molecular gas ring and the main disk.[16][15][17]

SN 2002fb

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Onesupernova has been observed in NGC 759,[18] SN 2002fb, which was discovered on September 6, 2002. It was classified as atype Ia supernova.[19][20][21]

See also

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References

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  1. ^abcdefghij"NASA/IPAC Extragalactic Database".Results for NGC 759. Retrieved2019-01-06.
  2. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2019-01-08.
  3. ^"New General Catalog Objects: NGC 750 – 799".cseligman.com. Retrieved2019-01-03.
  4. ^Giuricin, G.; Marinoni, C.; Ceriani, L.; Pisani, A. (November 2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups".The Astrophysical Journal.543 (1):178–194.arXiv:astro-ph/0001140.Bibcode:2000ApJ...543..178G.doi:10.1086/317070.ISSN 0004-637X.S2CID 9618325.
  5. ^Garcia, A. M. (1993-07-01). "General study of group membership. II – Determination of nearby groups".Astronomy and Astrophysics Supplement Series.100:47–90.Bibcode:1993A&AS..100...47G.ISSN 0365-0138.
  6. ^Fouque, P.; Gourgoulhon, E.; Chamaraux, P.; Paturel, G. (1992-05-01). "Groups of galaxies within 80 Mpc. II – The catalogue of groups and group members".Astronomy and Astrophysics Supplement Series.93:211–233.Bibcode:1992A&AS...93..211F.ISSN 0365-0138.
  7. ^"NGC 759".simbad. Retrieved2019-01-08.
  8. ^"Detailed Object Classifications".ned.ipac.caltech.edu. Retrieved2019-01-08.
  9. ^Righetti, G.; Giovannini, G.; Feretti, L. (1988-04-01). "WSRT observations at 327 MHz of the cluster A262".Astronomy and Astrophysics Supplement Series.73:173–179.Bibcode:1988A&AS...73..173R.ISSN 0365-0138.
  10. ^Zhao, Jun-Hui; Burns, Jack O.; Owen, Frazer N. (1989-07-01)."A 20 CM VLA survey of Abell clusters of galaxies. I – Distance class of not greater than 3 clusters".The Astronomical Journal.98:64–107.Bibcode:1989AJ.....98...64Z.doi:10.1086/115128.ISSN 0004-6256.
  11. ^Miller, Neal A.; Owen, Frazer N. (2001-06-01). "The Radio Galaxy Populations of Nearby Northern Abell Clusters".The Astrophysical Journal Supplement Series.134 (2):355–383.arXiv:astro-ph/0101114.Bibcode:2001ApJS..134..355M.doi:10.1086/320857.ISSN 0067-0049.S2CID 119052072.
  12. ^abFeretti, L.; Giovannini, G. (1994-01-01). "Structures of small-size radio galaxies in clusters".Astronomy and Astrophysics.281:375–387.Bibcode:1994A&A...281..375F.ISSN 0004-6361.
  13. ^abVila-Vilaró, B.; Cepa, J.; Butner, H. M. (2003-09-01)."CO (3–2) Observations of Early-Type Galaxies with the Heinrich Hertz Telescope".The Astrophysical Journal.594 (1):232–246.Bibcode:2003ApJ...594..232V.doi:10.1086/376775.ISSN 0004-637X.
  14. ^Wegner, G. A.; Corsini, E. M.; Thomas, J.; Saglia, R. P.; Bender, R.; Pu, S. B. (2012)."Further Evidence for Large Central Mass-to-light Ratios in Early-type Galaxies: The Case of Ellipticals and Lenticulars in the A262 Cluster".The Astronomical Journal.144 (3): 78.arXiv:1206.5768.Bibcode:2012AJ....144...78W.doi:10.1088/0004-6256/144/3/78.hdl:11577/2526313.ISSN 1538-3881.S2CID 118679035.
  15. ^abcdWiklind, T.; Combes, F.; Henkel, C.; Wyrowski, F. (1997-07-01). "Molecular gas in the elliptical galaxy NGC 759. Interferometric CO observations".Astronomy and Astrophysics.323:727–738.arXiv:astro-ph/9702080.Bibcode:1997A&A...323..727W.ISSN 0004-6361.
  16. ^abcdVlasyuk, V. V.; Sil'chenko, O. K. (2000-02-01). "NGC 759: A giant elliptical with a just-forming decoupled nucleus".Astronomy and Astrophysics.354:28–34.Bibcode:2000A&A...354...28V.ISSN 0004-6361.
  17. ^abcLeeuw, Lerothodi L.; Davidson, Jacqueline; Dowell, C. Darren; Matthews, Henry E. (2008)."Spatially Resolved Imaging at 350 μm of Cold Dust in Nearby Elliptical Galaxies".The Astrophysical Journal.677 (1): 249.arXiv:0801.0591.Bibcode:2008ApJ...677..249L.doi:10.1086/528838.ISSN 0004-637X.S2CID 14316328.
  18. ^"List of supernovae sorted by host name".Bright Supernova – Archives. Retrieved2019-01-03.
  19. ^"Bright Supernovae – 2002".rochesterastronomy.org. Retrieved2019-01-11.
  20. ^"2002fb – The Open Supernova Catalog". Archived fromthe original on 2016-09-17. Retrieved2019-01-11.
  21. ^"SN 2002fb | Transient Name Server".wis-tns.weizmann.ac.il. Retrieved2019-01-11.

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