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UGC 6614

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Giant spiral galaxy
UGC 6614
The LSB galaxy UGC 6614, imaged by theHubble Space Telescope
Observation data (J2000epoch)
ConstellationLeo
Right ascension11h 39m 14.9s[1]
Declination17° 08′ 37″[1]
Redshift0.021188 ± 0.000007[1]
Heliocentric radial velocity6,359 ± 2km/s
Distance322Mly (98.72Mpc)
Apparent magnitude (V)14.377[1]
Absolute magnitude (B)-22.00 ± 0.50[1]
Characteristics
Type(R)SA(r)a[1]
Size~309,000 ly (94.75 kpc) (estimated)[1]
Apparent size (V)1.7' × 1.4'[1]
Other designations
2MASX J11391484+1708368,MCG +03-30-029,PGC 36122,CGCG 097-40[1]

UGC 6614 is a giantspiral galaxy located about 330 millionlight-years away in theconstellationLeo. It has an estimated diameter of nearly 300,000 light-years.[2]

Physical characteristics

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UGC 6614 is classified as alow surface brightness (LSB) galaxy.[3][4][5] The galaxy is nearly face-on and has a ring-like feature around itsbulge,[6] with distinctive extendedspiral arms.[7] The bulge of UGC 6614 is found to be red, similar to those of S0 and otherelliptical galaxies, hinting at the existence of an oldstar population.[8] In its center,globular clusters are present.[9]

It is hypothesised UGC 6614 might be a giant elliptical galaxy, but because of repeatedmergers with otherdisk galaxies, it shows a stellar disk structure, causing its spiral-like appearance.[10]

UGC 6614 possibly shows the highestmetallicity known for an LSB galaxy with an estimated log value of (O/H) 1⁄4 3 to 2.84.[11] Its nucleus showsAGN activity at optical wavelengths[12] and appears as a bright core in X-ray emission, according toXMM-Newton archival data.[4]

Black hole

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UGC 6614 contains asupermassive black hole in its center, estimated at 3.8 millionsolar masses.[13]

Unconfirmed Supernova

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AT 2020ojw, anastronomical transient, was discovered in UGC 6614 in July 2020 byATLAS (Asteroid Terrestrial-impact Last Alert System). It had amagnitude of 18.4 and is a candidatesupernova.[14][15]

Group Membership

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UGC 6614 is a member of a small group of 3 galaxies known as [T2015] nest 100958. [T2015] nest 100958 has a velocity dispersion of 244 km/s and an estimated mass of 1.38 × 1013M. Other members of the group include its brightest member,NGC 3767, andCGCG 097-024.[16] The group is part of theComa Supercluster.[17][18][19]

See also

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References

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  1. ^abcdefghi"NASA/IPAC Extragalactic Database".Results for UGC 6614. Retrieved2017-07-22.
  2. ^"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2024-08-10.
  3. ^"Giant Low Surface Brightness Galaxies - Ronald J. Buta".ned.ipac.caltech.edu. Retrieved2024-08-09.
  4. ^abNaik, Sachindra; Das, M.; Jain, C.; Paul, B. (March 2010)."An X-ray bright nucleus in the low-surface-brightness galaxy UGC 6614".Monthly Notices of the Royal Astronomical Society.404 (4): 2056.arXiv:1001.5096.Bibcode:2010MNRAS.404.2056N.doi:10.1111/j.1365-2966.2010.16423.x.ISSN 0035-8711.
  5. ^Mishra, Alka; Kantharia, N. G.; Das, M.; Omar, A.; Srivastava, D. C. (2017-01-21)."GMRT HI study of giant low surface brightness galaxies".Monthly Notices of the Royal Astronomical Society.464 (3):2741–2751.arXiv:1609.07544.doi:10.1093/mnras/stw2506.ISSN 0035-8711.
  6. ^Hinz, J. L.; Rieke, M. J.; Rieke, G. H.; Willmer, C. N. A.; Misselt, K.; Engelbracht, C. W.; Blaylock, M.; Pickering, T. E. (2007-07-01)."Spitzer Observations of Low-Luminosity Isolated and Low Surface Brightness Galaxies".The Astrophysical Journal.663 (2):895–907.arXiv:0704.2059.Bibcode:2007ApJ...663..895H.doi:10.1086/518817.ISSN 0004-637X.
  7. ^Mehta, Kushal T.; O'Neil, K. (2006-12-01)."Mapping a Low Surface Brightness Galaxy".American Astronomical Society Meeting Abstracts.209: 04.11.Bibcode:2006AAS...209.0411M.
  8. ^Quillen, A. C.; Pickering, T. E. (1997-05-01). "Evidence for Old Stars in the Red Low Surface Brightness Galaxies UGC 6614 and F568-6".arXiv:astro-ph/9705115.
  9. ^Kim, J. H.; McGaugh, S. S. (2002-12-01)."Hubble Space Telescope Imaging of Globular Clusters in the Face-on Galaxies UGC 5981 & UGC 6614".American Astronomical Society Meeting Abstracts.201: 13.04.Bibcode:2002AAS...201.1304K.
  10. ^Yoachim, Peter; Schmitz, D.; Loebman, S.; Debattista, V. P.; Kwak, S. (2014-01-01)."IFU Observations of Giant Low Surface Brightness Galaxies".American Astronomical Society Meeting Abstracts #223.223: 453.05.Bibcode:2014AAS...22345305Y.
  11. ^McGaugh, S.S. (1994)."Oxygen Abundances In Low Surface Brightness Disk Galaxies".The Astrophysical Journal.426: 135.arXiv:astro-ph/9311064.Bibcode:1994ApJ...426..135M.doi:10.1086/174049. Retrieved2024-08-09.
  12. ^Schombert, J. (1998-10-01)."Active Galactic Nucleus Activity in Giant, Low Surface Brightness Galaxies".The Astronomical Journal.116 (4):1650–1656.Bibcode:1998AJ....116.1650S.doi:10.1086/300558.ISSN 0004-6256.
  13. ^Ramya, S.; Prabhu, T. P.; Das, M. (2011-12-01)."Active galactic nucleus activity and black hole masses in low surface brightness galaxies".Monthly Notices of the Royal Astronomical Society.418 (2):789–800.arXiv:1108.0763.Bibcode:2011MNRAS.418..789R.doi:10.1111/j.1365-2966.2011.19530.x.ISSN 0035-8711.
  14. ^Srivastav, S.; Smith, K. W.; McBrien, O.; Smartt, S. J.; Gillanders, J.; Clark, P.; Fulton, M.; O'Neill, D.; Young, D. R.; McCollum, M.; Townsend, A.; Chen, T. W.; Anderson, J.; Denneau, L.; Flewelling, H. (2020-07-01)."ATLAS20sgz (AT2020ojw): discovery of a candidate supernova in UGC 6614 (93 Mpc)".Transient Name Server AstroNote.135: 1.Bibcode:2020TNSAN.135....1S.
  15. ^"AT 2020ojw | Transient Name Server".www.wis-tns.org. Retrieved2024-08-09.
  16. ^Tully, R. Brent (2015-05-01)."Galaxy Groups: A 2MASS Catalog".The Astronomical Journal.149 (5): 171.arXiv:1503.03134.Bibcode:2015AJ....149..171T.doi:10.1088/0004-6256/149/5/171.ISSN 0004-6256.
  17. ^"UGC 6614".simbad.cds.unistra.fr. Retrieved2024-08-30.
  18. ^Mahajan, Smriti; Singh, Ankit; Shobhana, Devika (2018-08-01)."Ultraviolet and optical view of galaxies in the Coma supercluster".Monthly Notices of the Royal Astronomical Society.478 (4):4336–4347.arXiv:1805.09029.Bibcode:2018MNRAS.478.4336M.doi:10.1093/mnras/sty1370.ISSN 0035-8711.
  19. ^Gregory, S. A.; Thompson, L. A. (1978-06-01)."The Coma/A1367 supercluster and its environs".The Astrophysical Journal.222:784–799.Bibcode:1978ApJ...222..784G.doi:10.1086/156198.ISSN 0004-637X.
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External links

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