ngc+1271 Latitude and Longitude:

Sky map 03h 19m 11.3s, 41° 21′ 12″
From Wikipedia, the free encyclopedia
NGC 1271
SDSS image of NGC 1271
Observation data ( J2000 epoch)
Constellation Perseus
Right ascension03h 19m 11.3s [1]
Declination41° 21′ 12″ [1]
Redshift0.019183 [1]
Heliocentric radial velocity5751 km/s [1]
Distance249  Mly (76.3  Mpc) [1]
Group or cluster Perseus Cluster
Apparent magnitude (V)15.1 [1]
Characteristics
TypeE/SO [2]
Mass/Light ratio1.35 [3]  M/ L
Size~14,000  ly (4.4  kpc) (estimated) [3]
Apparent size (V)0.567 x 0.306 [1]
Other designations
CGCG 540-96, PGC 12367 [1]

NGC 1271 is a compact elliptical or lenticular galaxy [2] located about 250 million light-years away [4] in the constellation Perseus. [5] The galaxy was discovered by astronomer Guillaume Bigourdan on November 14, 1884. [6] NGC 1271 is a member of the Perseus Cluster [7] [6] and has a nuclear dust disk in its center. [3] It also has an edge-on, intermediate-scale disk and has a central bulge. [2] Like NGC 1277, NGC 1271 is a candidate " relic galaxy". [8]

Supermassive black hole

Using orbital-based stellar dynamical models, Walsh et al. determined that the supermassive black hole in the center of NGC 1271 has a mass of 3.0+1.0
−1.1
×109  M
. [3]

See also

References

  1. ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 1271. Retrieved 2018-06-20.
  2. ^ a b c Graham, Alister W.; Ciambur, Bogdan C.; Savorgnan, Giulia A. D. (2016). "Disky Elliptical Galaxies and the Allegedly Over-massive Black Hole in the Compact "ES" Galaxy NGC 1271". The Astrophysical Journal. 831 (2): 132. arXiv: 1608.00711. Bibcode: 2016ApJ...831..132G. doi: 10.3847/0004-637X/831/2/132. ISSN  0004-637X. S2CID  118435675.
  3. ^ a b c d Walsh, Jonelle L.; Bosch, Remco C. E. van den; Gebhardt, Karl; Yildirim, Akin; Gültekin, Kayhan; Husemann, Bernd; Richstone, Douglas O. (2015-08-03). "The Black Hole in the Compact, High-Dispersion Galaxy NGC 1271". The Astrophysical Journal. 808 (2): 183. arXiv: 1506.05129. Bibcode: 2015ApJ...808..183W. doi: 10.1088/0004-637X/808/2/183. ISSN  1538-4357. S2CID  41570998.
  4. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-06-23.
  5. ^ "Revised NGC Data for NGC 1271". spider.seds.org. Retrieved 2018-06-23.
  6. ^ a b "New General Catalog Objects: NGC 1250 - 1299". cseligman.com. Retrieved 2018-06-15.
  7. ^ Brunzendorf, J.; Meusinger, H. (October 1, 1999). "The galaxy cluster Abell 426 (Perseus). A catalogue of 660 galaxy positions, isophotal magnitudes and morphological types". Astronomy and Astrophysics Supplement Series. 139 (1): 141–161. Bibcode: 1999A&AS..139..141B. doi: 10.1051/aas:1999111. ISSN  0365-0138.
  8. ^ Ferré-Mateu, Anna; Mezcua, Mar; Trujillo, Ignacio; Balcells, Marc; Bosch, Remco C. E. van den (2015). "Massive Relic Galaxies Challenge the Co-evolution of Super-massive Black Holes and Their Host Galaxies". The Astrophysical Journal. 808 (1): 79. arXiv: 1506.02663. Bibcode: 2015ApJ...808...79F. doi: 10.1088/0004-637X/808/1/79. ISSN  0004-637X. S2CID  118777377.

ngc+1271 Latitude and Longitude:

Sky map 03h 19m 11.3s, 41° 21′ 12″
From Wikipedia, the free encyclopedia
NGC 1271
SDSS image of NGC 1271
Observation data ( J2000 epoch)
Constellation Perseus
Right ascension03h 19m 11.3s [1]
Declination41° 21′ 12″ [1]
Redshift0.019183 [1]
Heliocentric radial velocity5751 km/s [1]
Distance249  Mly (76.3  Mpc) [1]
Group or cluster Perseus Cluster
Apparent magnitude (V)15.1 [1]
Characteristics
TypeE/SO [2]
Mass/Light ratio1.35 [3]  M/ L
Size~14,000  ly (4.4  kpc) (estimated) [3]
Apparent size (V)0.567 x 0.306 [1]
Other designations
CGCG 540-96, PGC 12367 [1]

NGC 1271 is a compact elliptical or lenticular galaxy [2] located about 250 million light-years away [4] in the constellation Perseus. [5] The galaxy was discovered by astronomer Guillaume Bigourdan on November 14, 1884. [6] NGC 1271 is a member of the Perseus Cluster [7] [6] and has a nuclear dust disk in its center. [3] It also has an edge-on, intermediate-scale disk and has a central bulge. [2] Like NGC 1277, NGC 1271 is a candidate " relic galaxy". [8]

Supermassive black hole

Using orbital-based stellar dynamical models, Walsh et al. determined that the supermassive black hole in the center of NGC 1271 has a mass of 3.0+1.0
−1.1
×109  M
. [3]

See also

References

  1. ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 1271. Retrieved 2018-06-20.
  2. ^ a b c Graham, Alister W.; Ciambur, Bogdan C.; Savorgnan, Giulia A. D. (2016). "Disky Elliptical Galaxies and the Allegedly Over-massive Black Hole in the Compact "ES" Galaxy NGC 1271". The Astrophysical Journal. 831 (2): 132. arXiv: 1608.00711. Bibcode: 2016ApJ...831..132G. doi: 10.3847/0004-637X/831/2/132. ISSN  0004-637X. S2CID  118435675.
  3. ^ a b c d Walsh, Jonelle L.; Bosch, Remco C. E. van den; Gebhardt, Karl; Yildirim, Akin; Gültekin, Kayhan; Husemann, Bernd; Richstone, Douglas O. (2015-08-03). "The Black Hole in the Compact, High-Dispersion Galaxy NGC 1271". The Astrophysical Journal. 808 (2): 183. arXiv: 1506.05129. Bibcode: 2015ApJ...808..183W. doi: 10.1088/0004-637X/808/2/183. ISSN  1538-4357. S2CID  41570998.
  4. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-06-23.
  5. ^ "Revised NGC Data for NGC 1271". spider.seds.org. Retrieved 2018-06-23.
  6. ^ a b "New General Catalog Objects: NGC 1250 - 1299". cseligman.com. Retrieved 2018-06-15.
  7. ^ Brunzendorf, J.; Meusinger, H. (October 1, 1999). "The galaxy cluster Abell 426 (Perseus). A catalogue of 660 galaxy positions, isophotal magnitudes and morphological types". Astronomy and Astrophysics Supplement Series. 139 (1): 141–161. Bibcode: 1999A&AS..139..141B. doi: 10.1051/aas:1999111. ISSN  0365-0138.
  8. ^ Ferré-Mateu, Anna; Mezcua, Mar; Trujillo, Ignacio; Balcells, Marc; Bosch, Remco C. E. van den (2015). "Massive Relic Galaxies Challenge the Co-evolution of Super-massive Black Holes and Their Host Galaxies". The Astrophysical Journal. 808 (1): 79. arXiv: 1506.02663. Bibcode: 2015ApJ...808...79F. doi: 10.1088/0004-637X/808/1/79. ISSN  0004-637X. S2CID  118777377.

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