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NGC 753

Coordinates:Sky map01h 57m 42.2104s, +35° 54′ 58.262″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Andromeda
NGC 753
NGC 753 imaged byPanSTARRS
Observation data (J2000epoch)
ConstellationAndromeda
Right ascension01h 57m 42.2104s[1]
Declination+35° 54′ 58.262″[1]
Redshift0.016221[1]
Heliocentric radial velocity4863 km/s[1]
Distance220 Mly (67 Mpc)[2]
Group orclusterAbell 262
Apparent magnitude (V)12.97[1]
Characteristics
TypeSAB(rs)bc[1]
Size~148,000 ly (45.39 kpc) (estimated)[1]
Apparent size (V)2.5′ × 1.9′[1]
Other designations
IRAS 01547+3540,UGC 1437,MCG +06-05-066,PGC 7387,CGCG 522-086[1]

NGC 753 is aspiral galaxy[1] located 220 millionlight-years away[2] in theconstellationAndromeda. The galaxy was discovered by astronomer byHeinrich d'Arrest on September 16, 1865[3] and is a member ofAbell 262.[4][5][6][7][8][9]

NGC 753 has roughly 2-3 times more mass than theMilky Way[4] and is classified as aradio galaxy.[10][11][12]

Physical characteristics

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NGC 753 contains two main arms that extend to 180° on either side of the galaxy.[13][14] From the two main arms, there are three larger and weaker arms that sub-divide into several branches.[13] This open structure of the arms may be due to the influence ofNGC 759 which is a close companion of NGC 753[13][14] that lies 1.4 Mly (0.44 Mpc) away.[14]

Supermassive black hole

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NGC 753 has asupermassive black hole with an estimated mass of (2.2 ± 0.4) × 107M☉.[15]

Supernovae

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NGC 753 has hosted twosupernovae:[16]

  • SN 1954E (type unknown, mag. 18.5) was discovered byFritz Zwicky on 26 September 1954.[17][18][16][19]
  • SN 2025mbr (Type Ia, mag. 17.3695) was discovered by theAutomatic Learning for the Rapid Classification of Events (ALeRCE) on 25 May 2025.[20]

See also

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References

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  1. ^abcdefghij"Results for object NGC 0753".NASA/IPAC Extragalactic Database.NASA andCaltech. Retrieved2019-01-03.
  2. ^abPilyugin, L. S.; Grebel, E. K.; Kniazev, A. Y. (2014)."The Abundance Properties of Nearby Late-type Galaxies. I. The Data".The Astronomical Journal.147 (6): 131.arXiv:1403.5461.Bibcode:2014AJ....147..131P.doi:10.1088/0004-6256/147/6/131.ISSN 1538-3881.S2CID 119239041.
  3. ^"New General Catalog Objects: NGC 750 - 799".cseligman.com. Retrieved2019-01-03.
  4. ^abHenry, R. B. C.; Balkowski, C.; Cayatte, V.; Edmunds, M. G.; Pagel, B. E. J. (1996-12-01)."The effects of cluster environment on the chemical evolution of galaxies. III. NGC 753".Monthly Notices of the Royal Astronomical Society.283 (2):635–647.Bibcode:1996MNRAS.283..635H.doi:10.1093/mnras/283.2.635.ISSN 0035-8711.
  5. ^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.
  6. ^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.
  7. ^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.
  8. ^"NGC 753".sim-id. Retrieved2019-01-03.
  9. ^"Detailed Object Classifications".ned.ipac.caltech.edu. Retrieved2019-01-03.
  10. ^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.
  11. ^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.
  12. ^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.
  13. ^abcdel Rio, M. S.; Cepa, J. (1998-12-01). "The nature of arms in spiral galaxies. III. Azimuthal profiles".Astronomy and Astrophysics.340:1–20.Bibcode:1998A&A...340....1D.ISSN 0004-6361.
  14. ^abcdel Río, M. S.; Cepa, J. (1999-01-01)."The nature of arms in spiral galaxies. IV. Symmetries and asymmetries".Astronomy and Astrophysics Supplement Series.134 (2):333–358.Bibcode:1999A&AS..134..333D.doi:10.1051/aas:1999440.ISSN 0365-0138.
  15. ^Seigar, Marc S.; Kennefick, Daniel; Kennefick, Julia; Lacy, Claud H. S. (2008-05-10). "Discovery of a relationship between spiral arm morphology and supermassive black hole mass in disk galaxies".The Astrophysical Journal.678 (2):L93–L96.arXiv:0804.0773.Bibcode:2008ApJ...678L..93S.doi:10.1086/588727.ISSN 0004-637X.S2CID 118430417.
  16. ^ab"List of supernovae sorted by host name".Bright Supernova - Archives. Retrieved2019-01-03.
  17. ^Kowal, C. T.; Sargent, W. L. W.; Zwicky, F. (1970-06-01)."The 1969 Palomar Supernova Search".Publications of the Astronomical Society of the Pacific.82 (487): 736.Bibcode:1970PASP...82..736K.doi:10.1086/128951.ISSN 0004-6280.
  18. ^"Other Supernovae images".rochesterastronomy.org. Retrieved2019-01-04.
  19. ^"1954E | Transient Name Server".wis-tns.weizmann.ac.il. Retrieved2019-01-04.
  20. ^"SN 2025mbr".Transient Name Server.IAU. Retrieved16 June 2025.

External links

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