NGC 4312

Last updated
NGC 4312
SDSS NGC 4312.jpg
SDSS image of NGC 4312.
Observation data (J2000 epoch)
Constellation Coma Berenices
Right ascension 12h 22m 31.3s [1]
Declination 15° 32′ 17″ [1]
Redshift 0.000510 [1]
Helio radial velocity 153 km/s [1]
Distance 55  Mly (17  Mpc) [2]
Group or cluster Virgo Cluster
Apparent magnitude  (V)12.53 [1]
Characteristics
Type SA(rs)ab [1]
Size~59,000  ly (18  kpc) (estimated) [1]
Apparent size  (V)4.6 x 1.1 [1]
Other designations
UGC 07442, VCC 0559, PGC 040095, MCG +03-32-014 [1]

NGC 4312 is an edge-on unbarred spiral galaxy [3] located about 55 million light-years away [2] in the constellation Coma Berenices. It was discovered by astronomer William Herschel on January 14, 1787. [4] NGC 4312 is a member of the Virgo Cluster [5] [6] [7] and is a LINER galaxy. [8]

Contents

It has undergone ram-pressure stripping in the past. [9]

Black Hole

NGC 4312 may harbor an intermediate-mass black hole with an estimated mass ranging from 10,000 (1*10^4) to 300,000 (3*10^5) solar masses. [10]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 4457</span> Spiral galaxy in the constellation of Virgo

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<span class="mw-page-title-main">NGC 4607</span> Edge-on spiral galaxy in the constellation Virgo

NGC 4607 is an edge-on spiral galaxy located about 56 million light-years away in the constellation Virgo. NGC 4607 was discovered by astronomer R. J. Mitchell on April 24, 1854. The galaxy is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4638</span> Lenticular galaxy in the constellation Virgo

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<span class="mw-page-title-main">Coma I</span> Galaxy cluster in constellation Coma Berenices

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<span class="mw-page-title-main">NGC 3821</span> Spiral galaxy in the constellation Leo

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

NGC 4212 is a flocculent spiral galaxy with LINER activity located about 53 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 8, 1784 and was listed in the NGC catalog as NGC 4208. He then observed the same galaxy and listed it as NGC 4212. Astronomer John Louis Emil Dreyer later concluded that NGC 4208 was identical to NGC 4212. NGC 4212 is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4237</span> Flocculent spiral galaxy in the constellation Coma Berenices

NGC 4237 is a flocculent spiral galaxy located about 60 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on December 30, 1783 and is a member of the Virgo Cluster. It is also classified as a LINER galaxy and as a Seyfert galaxy.

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

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

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<span class="mw-page-title-main">NGC 4065 Group</span> Group of galaxies in the constellation of Coma Berenices

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<span class="mw-page-title-main">NGC 4294</span> Flocculent barred spiral 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 4298</span> Flocculent spiral galaxy in the constellation Coma Berenices

NGC 4298 is a flocculent spiral galaxy located about 53 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 8, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4299</span> Relatively featureless 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 4302</span> Edge-on spiral galaxy in the constellation Coma Berenices

NGC 4302 is an edge-on spiral galaxy located about 55 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 8, 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 4313</span> Spiral galaxy in the constellation Virgo

NGC 4313 is an edge-on spiral galaxy located about 50 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on March 15, 1784. NGC 4313 is a member of the Virgo Cluster and is classified as LINER and as a Seyfert galaxy.

<span class="mw-page-title-main">NGC 4316</span> Spiral galaxy in the constellation Virgo

NGC 4316 is an edge-on spiral galaxy located about 70 million light-years away in the constellation Virgo. It was discovered by astronomer Wilhelm Tempel on March 17, 1882. NGC 4316 is a member of the Virgo Cluster and is classified as LINER and as a Seyfert galaxy.

<span class="mw-page-title-main">NGC 4324</span> Lenticular 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 4312. Retrieved 2019-08-22.
  2. 1 2 Hughes, T. M.; Boissier, S.; Buat, V.; Ciesla, L.; Gavazzi, G.; Fossati, M.; Boselli, A. (2015-07-01). "Hα imaging of the Herschel Reference Survey - The star formation properties of a volume-limited, K-band-selected sample of nearby late-type galaxies". Astronomy & Astrophysics. 579: A102. arXiv: 1504.01876 . Bibcode:2015A&A...579A.102B. doi: 10.1051/0004-6361/201525712 . ISSN   0004-6361.
  3. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2019-08-22.
  4. ↑ "New General Catalog Objects: NGC 4300 - 4349". cseligman.com. Retrieved 2019-08-19.
  5. ↑ Binggeli, B.; Sandage, A.; Tammann, G. A. (1985-09-01). "Studies of the Virgo Cluster. II - A catalog of 2096 galaxies in the Virgo Cluster area". The Astronomical Journal. 90: 1681–1759. Bibcode:1985AJ.....90.1681B. doi:10.1086/113874. ISSN   0004-6256.
  6. ↑ Buta, Ronald J.; Sheth, Kartik; Athanassoula, E.; Bosma, A.; Knapen, Johan H.; Laurikainen, Eija; Salo, Heikki; Elmegreen, Debra; Ho, Luis C. (2015-04-01). "A Classical Morphological Analysis of Galaxies in the Spitzer Survey of Stellar Structure in Galaxies (S4G)". The Astrophysical Journal Supplement Series. 217 (2): 32. arXiv: 1501.00454 . Bibcode:2015ApJS..217...32B. doi:10.1088/0067-0049/217/2/32. ISSN   0067-0049. S2CID   119202943.
  7. ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2019-08-22.
  8. ↑ Colpi, M.; Bonfanti, C.; Boselli, A.; Cortese, L.; Arosio, I.; Gavazzi, G.; Decarli, R. (2007-07-06). "The census of nuclear activity of late-type galaxies in the Virgo cluster". Monthly Notices of the Royal Astronomical Society. 381 (1): 136–150. arXiv: 0707.0999 . Bibcode:2007MNRAS.381..136D. doi: 10.1111/j.1365-2966.2007.12208.x .
  9. ↑ Palous, J.; Taylor, R.; Jachym, P.; Koppen, J. (2018-06-15). "Ram Pressure Stripping Made Easy: An Analytical Approach". Monthly Notices of the Royal Astronomical Society. 479 (4): 4367–4390. arXiv: 1806.05887 . Bibcode:2018MNRAS.479.4367K. doi:10.1093/mnras/sty1610. S2CID   119245255.
  10. ↑ Davis, Benjamin L.; Soria, Roberto; Graham, Alister W. (2019). "Expected intermediate mass black holes in the Virgo cluster. II. Late-type galaxies". Monthly Notices of the Royal Astronomical Society. 484 (1): 814. arXiv: 1811.03232 . Bibcode:2019MNRAS.484..814G. doi:10.1093/mnras/sty3068. S2CID   119303249.
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