NGC 753

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NGC 753
PanSTARRS NGC 753.jpg
NGC 753 imaged by PanSTARRS
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 01h 57m 42.2104s [1]
Declination +35° 54′ 58.262″ [1]
Redshift 0.016221 [1]
Heliocentric radial velocity 4863 km/s [1]
Distance 220  Mly (67  Mpc) [2]
Group or cluster Abell 262
Apparent magnitude  (V)12.97 [1]
Characteristics
Type SAB(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 a spiral galaxy [1] located 220 million light-years away [2] in the constellation Andromeda. The galaxy was discovered by astronomer by Heinrich d'Arrest on September 16, 1865 [3] and is a member of Abell 262. [4] [5] [6] [7] [8] [9]

Contents

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

Physical characteristics

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 of NGC 759 which is a close companion of NGC 753 [13] [14] that lies 1.4  Mly (0.44  Mpc ) away. [14]

Supermassive black hole

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

Supernovae

NGC 753 has hosted two supernovae: [16]

See also

References

  1. 1 2 3 4 5 6 7 8 9 10 "Results for object NGC 0753". NASA/IPAC Extragalactic Database. NASA and Caltech . Retrieved 2019-01-03.
  2. 1 2 Pilyugin, 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. Retrieved 2019-01-03.
  4. 1 2 Henry, 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. Retrieved 2019-01-03.
  9. ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2019-01-03.
  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. 1 2 3 del 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. 1 2 3 del 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. 1 2 "List of supernovae sorted by host name". Bright Supernova - Archives. Retrieved 2019-01-03.
  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. Retrieved 2019-01-04.
  19. ↑ "1954E | Transient Name Server". wis-tns.weizmann.ac.il. Retrieved 2019-01-04.
  20. ↑ "SN 2025mbr". Transient Name Server. IAU . Retrieved 16 June 2025.
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