NGC 4876

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NGC 4876
SDSS NGC 4876.jpg
SDSS image of NGC 4876.
Observation data (J2000 epoch)
Constellation Coma Berenices
Right ascension 12h 59m 44.4s [1]
Declination 27° 54′ 45″ [1]
Redshift 0.022275 [1]
Helio radial velocity 6678 km/s [1]
Distance 325  Mly (99.5  Mpc) [1]
Group or cluster Coma Cluster
Apparent magnitude  (V)15.1 [1]
Characteristics
Type E5 [1]
Size~75,000  ly (23.00  kpc) (estimated) [1]
Apparent size  (V)0.58 x 0.40 [1]
Other designations
ARAK 398, CGCG 160-234, DRCG 27-124, MCG 5-31-73, PGC 44658 [1]

NGC 4876 is an elliptical galaxy [2] located about 325 million light-years away [3] in the constellation Coma Berenices. [4] NGC 4876 was discovered by astronomer Guillaume Bigourdan on May 16, 1885. [5] NGC 4876 is a member of the Coma Cluster. [6] [7]

Contents

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 4523</span> Spiral galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 4540</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 4659</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 4875</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 4886</span> Galaxy in the constellation Coma Berenices

NGC 4886 is an elliptical galaxy located about 327 million light-years away in the constellation Coma Berenices. NGC 4886 was discovered by astronomer Heinrich d'Arrest on April 6, 1864. It was then rediscovered by d'Arrest on April 22, 1865, and was listed as NGC 4882. NGC 4886 is a member of the Coma Cluster.

<span class="mw-page-title-main">NGC 4883</span> Galaxy in the constellation Coma Berenices

NGC 4883 is a barred lenticular galaxy located about 315 million light-years away in the constellation Coma Berenices. NGC 4883 was discovered by astronomer Heinrich d'Arrest on April 22, 1865. It is a member of the Coma Cluster.

<span class="mw-page-title-main">NGC 3816</span> Lenticular galaxy in the constellation Leo

NGC 3816 is a lenticular galaxy located about 270 million light-years away in the constellation Leo. It was discovered by astronomer Heinrich d'Arrest on May 9, 1864. NGC 3816 is a member of the Leo Cluster.

<span class="mw-page-title-main">NGC 3840</span> Spiral galaxy in the constellation Leo

NGC 3840 is a spiral galaxy located about 320 million light-years away in the constellation Leo. The galaxy was discovered by astronomer Heinrich d'Arrest on May 8, 1864. NGC 3840 is a member of the Leo Cluster. The galaxy is rich in neutral atomic hydrogen and is not interacting with its environment.

<span class="mw-page-title-main">NGC 3860</span> Spiral galaxy in the constellation Leo

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<span class="mw-page-title-main">NGC 4237</span> 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 4892</span> Galaxy in the constellation Coma Berenices

NGC 4892 is a spiral or lenticular galaxy with LINER activity located 275 million light-years away in the constellation Coma Berenices. It was discovered by the astronomer William Herschel on April 11, 1785, and is a member of the Coma Cluster.

<span class="mw-page-title-main">NGC 4060</span> Lenticular and LINER galaxy in the constellation Coma Berenices

NGC 4060 is a lenticular galaxy located 320 million light-years away in the constellation Coma Berenices. It was discovered by astronomer Albert Marth on March 18, 1865 and is a member of the NGC 4065 Group which is part of the Coma Supercluster.

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

NGC 4065 is an elliptical galaxy located 300 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 27, 1785. It was then rediscovered by John Herschel on April 29, 1832 and was listed as NGC 4057. NGC 4065 is the brightest member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4066</span> Galaxy in the constellation Coma Berenices

NGC 4066 is an elliptical galaxy located 340 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 27, 1785. NGC 4066 is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4072</span> Galaxy in the constellation Coma Berenices

NGC 4072 is a lenticular galaxy located 300 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer Ralph Copeland on April 3, 1872 and is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4393</span> Galaxy in the constellation of Coma Berenices

NGC 4393 is a spiral galaxy about 46 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 11, 1785. It is a member of the NGC 4274 Group, which is part of the Coma I Group or Cloud.

References

  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 4876. Retrieved 2018-04-18.
  2. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-04-18.
  3. ↑ "NED Query Results for NGC 4876". ned.ipac.caltech.edu. Retrieved 2018-04-19.
  4. ↑ "Revised NGC Data for NGC 4876". spider.seds.org. Retrieved 2018-04-18.
  5. ↑ "New General Catalog Objects: NGC 4850 - 4899". cseligman.com. Retrieved 2018-04-18.
  6. ↑ Kuntschner, Harald; Lucey, John R.; Smith, Russell J.; Hudson, Michael J.; Davies, Roger L. (2001-05-21). "On the dependence of spectroscopic indices of early-type galaxies on age, metallicity and velocity dispersion". Monthly Notices of the Royal Astronomical Society. 323 (3): 615–629. arXiv: astro-ph/0011234 . Bibcode:2001MNRAS.323..615K. doi:10.1046/j.1365-8711.2001.04263.x. ISSN   0035-8711. S2CID   15162556.
  7. ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-04-19.


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