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NGC 3504

Coordinates:Sky map11h 03m 11.2s, +27° 58′ 21″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Leo Minor
NGC 3504
Observation data (J2000epoch)
ConstellationLeo Minor
Right ascension11h 03m 11.2s[1]
Declination+27° 58′ 21″[1]
Redshift1534 ± 2 km/s[1]
Apparent magnitude (V)11.67[1]
Characteristics
Type(R)SAB(s)ab[1]
Apparent size (V)2.7 × 2.1[1]
Other designations
UGC 6118,MCG +05-26-039,PGC 33371[2]

NGC 3504 is abarred spiral galaxy in theconstellationLeo Minor. It has aHubble distance corresponding to 88 millionlight-years[3] and was discovered byWilliam Herschel in 1785.[4]

The luminosity class of NGC 3504 is I-II, with a broadHI line containing regions of ionizedhydrogen. Additionally, it is classfied as astarburst galaxy.[5]

There is a large amount of molecular gas centered on the galactic nucleus. Compared with other barred spiral galaxies, NGC 3504 is in an early phase of its evolution.[6]

Morphology

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NGC 3504 is classified as a type (R1')SAB(rs)ab galaxy.[7][8] It has a bright point-like nucleus embedded inside itsgalactic budge that is crossed by a thin bar. It hasspiral arms found wrapping around its inner ring which then peels off to form an outer, brokenpseudo-ring. The galaxy shows little evidence ofstar formation.[9]

Star-forming disk

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According toHubble Space Telescope, a star-forming disk has been found around the nucleus of NGC 3504, which the size of the disk'saxis is estimated to be 200 pc (~650light years).[10]

Mass

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The mass of NGC 3504 has been difficult to narrow down, but it is believed to be between 2.5*109 M⊙ and 9*109 M⊙.[11]

Supermassive black hole

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Thesupermassive black hole in NGC 3504 is estimated to be 107.8M○ (or 63 million solar masses), according tonear-infrared K-band brightness measurements for the galaxy's budge.[12]

Supernovae

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Twosupernovae have been observed in NGC 3504:

NGC 3504 group

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NGC 3504 is the brightest member of theNGC 3504 Group (also known asLGG 227), which is a member of theLeo II Groups, a series of galaxies andgalaxy clusters strung out from the right edge of theVirgo Supercluster.[18] There are eight other galaxies in the group includingNGC 3380,NGC 3400,NGC 3414,NGC 3451,NGC 3512, UGC 5921 and UGC 5958.[19] This NGC 3504 group is also mentioned by Abraham Mahtessian in his research paper published in 1998.[20]

References

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  1. ^abcdef"NASA/IPAC Extragalactic Database".Results for NGC 3504. Retrieved2008-04-10.
  2. ^"NGC 3504".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2021-02-23.
  3. ^"Results for NGC 3504".ned.ipac.caltech.edu. Retrieved2024-07-25.
  4. ^"New General Catalog Objects: NGC 3500 - 3549".cseligman.com. Retrieved2024-07-25.
  5. ^Balzano, V. A. (1983-05-01)."Star-burst galactic nuclei".The Astrophysical Journal.268:602–627.Bibcode:1983ApJ...268..602B.doi:10.1086/160983.ISSN 0004-637X.
  6. ^Franco, J & F, Ferrini (1993).Star Formation, Galaxies and the Interstellar Medium. Cambridge University Press.ISBN 978-0-521-44412-5.{{cite book}}: CS1 maint: multiple names: authors list (link)
  7. ^"Gérard de Vaucouleurs' Atlas of Galaxies".cseligman.com. Retrieved2024-07-25.
  8. ^"Galaxy Morphology of NGC 3504".kudzu.astr.ua.edu. Retrieved2024-07-25.
  9. ^de Jong, Roelof S. (1996),"Colour Gradients in the Optical and Near-IR",Spiral Galaxies in the Near-IR, ESO Astrophysics Symposia, Berlin, Heidelberg: Springer Berlin Heidelberg, pp. 43–47,doi:10.1007/978-3-540-49739-4_6,ISBN 978-3-662-22429-8, retrieved2024-07-25
  10. ^Comerón, S.; Knapen, J. H.; Beckman, J. E.; Laurikainen, E.; Salo, H.; Martínez-Valpuesta, I.; Buta, R. J. (March 2010)."AINUR: Atlas of Images of NUclear Rings".Monthly Notices of the Royal Astronomical Society.402 (4):2462–2490.arXiv:0908.0272.Bibcode:2010MNRAS.402.2462C.doi:10.1111/j.1365-2966.2009.16057.x.ISSN 0035-8711.
  11. ^Burbidge; et al. (1960)."The Rotation and Approximate Mass of NGC 3504".
  12. ^Dong, X. Y.; De Robertis, M. M. (March 2006)."Low-Luminosity Active Galaxies and Their Central Black Holes".The Astronomical Journal.131 (3):1236–1252.arXiv:astro-ph/0510694.Bibcode:2006AJ....131.1236D.doi:10.1086/499334.ISSN 0004-6256.
  13. ^Garnavich, P. (1998)."Supernova 1998cf in NGC 3504".International Astronomical Union Circular (6914): 1.Bibcode:1998IAUC.6914....1G.
  14. ^"SN 1998cf".Transient Name Server.IAU. Retrieved12 December 2024.
  15. ^Beckmann, S.; Li, W. D. (2001)."Supernova 2001ac in NGC 3504".International Astronomical Union Circular (7596): 1.Bibcode:2001IAUC.7596....1B.
  16. ^Matheson, T.; Jha, S.; Challis, P.; Kirshner, R.; Calkins, M. (2001). "Supernova 2001ac in NGC 3504".International Astronomical Union Circular (7597): 3.Bibcode:2001IAUC.7597....3M.
  17. ^"SN 2001ac".Transient Name Server.IAU. Retrieved12 December 2024.
  18. ^"The Leo III Groups".Atlas of the Universe.Archived from the original on July 22, 2012. Retrieved2010-11-27.
  19. ^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.
  20. ^Mahtessian, A. P. (1998-07-01)."Groups of galaxies. III. Some empirical characteristics".Astrophysics.41 (3):308–321.Bibcode:1998Ap.....41..308M.doi:10.1007/BF03036100.ISSN 0571-7256.

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