NGC 753

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NGC 753
PanSTARRS NGC 753.jpg
PanSTARRS image of NGC 753.
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 01h 57m 42.2s [1]
Declination 35° 54′ 58″ [1]
Redshift 0.016355 [1]
Helio radial velocity 4903 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~150,000  ly (46  kpc) (estimated) [1]
Apparent size  (V)2.5 x 1.9 [1]
Other designations
MCG 6-5-66, PGC 7387, UGC 1437 [1]

NGC 753 is a spiral galaxy [3] 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 [4] and is a member of Abell 262. [5] [6] [7] [8] [9] [10]

Contents

NGC 753 has roughly 2-3 times more mass than the Milky Way [5] and is classified as a radio galaxy. [11] [12] [13]

Physical characteristics

NGC 753 contains two main arms that extend to 180° on either side of the galaxy. [14] [15] From the two main arms, there are three larger and weaker arms that sub-divide into several branches. [14] This open structure of the arms may be due to the influence of NGC 759 which is a close companion of NGC 753 [14] [15] that lies 1.4  Mly (0.44  Mpc ) away. [15]

Supermassive black hole

NGC 753 has a supermassive black hole with an estimated mass of (2.2 ± 0.4) × 107 M☉. [16]

Supernovae

NGC 753 has hosted two supernovae, [17] SN 1954E which was discovered by Fritz Zwicky [18] [19] on September 26, 1954 [18] [19] [17] [20] and AT 2018ddf which was discovered on July 5, 2018. [17] [21] [22] Both supernovae were of unknown types. [17] [19] [21] [20] [22]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 3883</span> Galaxy in the constellation Leo

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<span class="mw-page-title-main">NGC 4212</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 3981</span> Spiral galaxy in the constellation Crater

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<span class="mw-page-title-main">NGC 708</span> Galaxy in the constellation Andromeda

NGC 708 is an elliptical galaxy located 240 million light-years away in the constellation Andromeda and was discovered by astronomer William Herschel on September 21, 1786. It is classified as a cD galaxy and is the brightest member of Abell 262. NGC 708 is a weak FR I radio galaxy and is also classified as a type 2 Seyfert galaxy.

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<span class="mw-page-title-main">NGC 669</span> Galaxy in the constellation Triangulum

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<span class="mw-page-title-main">NGC 679</span> Galaxy in the constellation Andromeda

NGC 679 is an elliptical or a lenticular galaxy located 210 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 13, 1784 and is a member of Abell 262.

<span class="mw-page-title-main">NGC 703</span> Galaxy in the constellation Andromeda

NGC 703 is a lenticular galaxy located 240 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786 and is also a member of Abell 262.

<span class="mw-page-title-main">NGC 705</span> Galaxy in the constellation Andromeda

NGC 705 is a lenticular galaxy located 240 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786 and is also a member of Abell 262.

<span class="mw-page-title-main">NGC 709</span> Galaxy in the constellation Andromeda

NGC 709 is a lenticular galaxy located 150 million light-years away in the constellation Andromeda. It was discovered by the Irish engineer and astronomer Bindon Blood Stoney on October 28, 1850 and is a member of the galaxy cluster Abell 262.

<span class="mw-page-title-main">NGC 710</span> Galaxy in the constellation Andromeda

NGC 710 is a spiral galaxy located 260 million light-years away in the constellation Andromeda. It was discovered by the Irish engineer and astronomer Bindon Blood Stoney on October 28, 1850 and is a member of the galaxy cluster Abell 262.

<span class="mw-page-title-main">NGC 759</span> Galaxy in the constellation Andromeda

NGC 759 is an elliptical galaxy located 230 million light-years away in the constellation Andromeda. NGC 759 was discovered by astronomer by Heinrich d'Arrest on September 17, 1865. It is a member of Abell 262.

<span class="mw-page-title-main">NGC 4076</span> Galaxy in the constellation Coma Berenices

NGC 4076 is a spiral galaxy located 290 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 27, 1785 and is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4294</span> Galaxy in the constellation Virgo

NGC 4294 is a barred spiral galaxy with flocculent spiral arms located about 55 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer William Herschel on March 15, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 7836</span> Galaxy in the constellation Andromeda

NGC 7836 is an irregular or spiral galaxy located about 260 million light-years away in the constellation of Andromeda. It was discovered by astronomer Lewis Swift on September 20, 1885.

<span class="mw-page-title-main">NGC 4299</span> Spiral galaxy in the constellation Virgo

NGC 4299 is a featureless spiral galaxy located about 55 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on March 15, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4307</span> Spiral galaxy in the constellation Virgo

NGC 4307 is an edge-on spiral galaxy located about 65 million light-years away in the constellation Virgo. It was discovered by astronomer Christian Peters in 1881 and is a member of the Virgo Cluster. It is also a LINER galaxy.

<span class="mw-page-title-main">NGC 4324</span> Galaxy in the constellation of Virgo

NGC 4324 is a lenticular galaxy located about 85 million light-years away in the constellation Virgo. It was discovered by astronomer Heinrich d'Arrest on March 4, 1862. NGC 4324 has a stellar mass of 5.62 × 1010M☉, and a baryonic mass of 5.88 × 1010M☉. The galaxy's total mass is around 5.25 × 1011M☉. NGC 4324 is notable for having a ring of star formation surrounding its nucleus. It was considered a member of the Virgo II Groups until 1999, when its distance was recalculated and it was placed in the Virgo W Group.

References

  1. 1 2 3 4 5 6 7 8 9 "NASA/IPAC Extragalactic Database". Results for NGC 753. 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. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-01-03.
  4. ↑ "New General Catalog Objects: NGC 750 - 799". cseligman.com. Retrieved 2019-01-03.
  5. 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.
  6. ↑ 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.
  7. ↑ 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.
  8. ↑ 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.
  9. ↑ "NGC 753". sim-id. Retrieved 2019-01-03.
  10. ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2019-01-03.
  11. ↑ 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.
  12. ↑ 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.
  13. ↑ 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.
  14. 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.
  15. 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.
  16. ↑ 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.
  17. 1 2 3 4 "List of supernovae sorted by host name". Bright Supernova - Archives. Retrieved 2019-01-03.
  18. 1 2 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.
  19. 1 2 3 "Other Supernovae images". rochesterastronomy.org. Retrieved 2019-01-04.
  20. 1 2 "1954E | Transient Name Server". wis-tns.weizmann.ac.il. Retrieved 2019-01-04.
  21. 1 2 "Bright Supernovae - 2018". rochesterastronomy.org. Retrieved 2019-01-04.
  22. 1 2 "AT 2018ddf | Transient Name Server". wis-tns.weizmann.ac.il. Retrieved 2019-01-04.


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