NGC 4709

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NGC 4709
2MASS NGC 4709.jpg
2MASS image of NGC 4709.
Observation data (J2000 epoch)
Constellation Centaurus
Right ascension 12h 50m 03.9s [1]
Declination −41° 22′ 55″ [1]
Redshift 0.015604 [1]
Helio radial velocity 4678 km/s [1]
Distance 150  Mly (45  Mpc) [2]
Group or cluster Centaurus Cluster (Cen 45 subgroup)
Apparent magnitude  (V)12.0 [1]
Characteristics
Type E1 [1]
Size~127,700  ly (39.14  kpc) (estimated) [1]
Apparent size  (V)2.4 x 2.0 [1]
Other designations
ESO 323-3, CCC 130, MCG -7-26-56, PGC 43423 [1]

NGC 4709 is an elliptical galaxy [3] located in the constellation Centaurus. [4] It is considered to be a member of the Centaurus Cluster [5] [6] and is the dominant member of a small group of galaxies known as "Cen 45" [7] which is currently merging with the main Centaurus Cluster (Cen 30) [8] even though the two subclusters' line of sight redshift velocities differ by about 1500 km/s. [9] NGC 4709 was discovered by astronomer James Dunlop on May 7, 1826. [10]

Contents

Distance estimates

Lucey et al. suggests that NGC 4709 and the Cen 45 subgroup lie at about the same distance as the main Centaurus Cluster [11] [8] which is about 150  Mly (45  Mpc ). [2]

See also

Related Research Articles

The Centaurus Cluster (A3526) is a cluster of hundreds of galaxies, located approximately 170 million light-years away in the Centaurus constellation. The brightest member galaxy is the elliptical galaxy NGC 4696 (~11m). The Centaurus cluster shares its supercluster, the Hydra–Centaurus Supercluster, with IC4329 Cluster and Hydra Cluster.

<span class="mw-page-title-main">NGC 4309</span> Lenticular galaxy in the constellation Virgo

NGC 4309 is a lenticular galaxy located about 55 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer Christian Peters in 1881 and is a member of the Virgo Cluster.

The Pavo–Indus Supercluster is a neighboring supercluster located about 60–70 Mpc (196–228 Mly) away in the constellations of Pavo, Indus, and Telescopium. The supercluster contains three main clusters, Abell 3656, Abell 3698, and Abell 3742.

<span class="mw-page-title-main">NGC 4570</span> Edge-on lenticular galaxy in the constellation Virgo

NGC 4570 is an edge-on lenticular galaxy located about 57 million light-years away in the constellation Virgo. NGC 4570 was discovered by astronomer William Herschel on April 13, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4596</span> Barred lenticular galaxy in the constellation Virgo

NGC 4596 is a barred lenticular galaxy located about 55 million light-years away in the constellation Virgo. NGC 4596 was discovered by astronomer William Herschel on March 15, 1784. NGC 4596 is a member of the Virgo Cluster and has an inclination of about 38°.

<span class="mw-page-title-main">NGC 4876</span> Elliptical galaxy in the constellation Coma Berenices

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

<span class="mw-page-title-main">NGC 1281</span> Elliptical galaxy in the constellation Perseus

NGC 1281 is a compact elliptical galaxy located about 200 million light-years away in the constellation Perseus. NGC 1281 was discovered by astronomer John Dreyer on December 12, 1876. It is a member of the Perseus Cluster.

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

NGC 3860 is a spiral galaxy located about 340 million light-years away in the constellation Leo. NGC 3860 was discovered by astronomer William Herschel on April 27, 1785. The galaxy is a member of the Leo Cluster and is a low-luminosity AGN (LLAGN). Gavazzi et al. however classified NGC 3860 as a strong AGN which may have been triggered by a supermassive black hole in the center of the galaxy.

<span class="mw-page-title-main">NGC 709</span> Lenticular 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 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> Elliptical 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 4070</span> Elliptical galaxy in the constellation Coma Berenices

NGC 4070 is an elliptical galaxy located 340 million light-years away in the constellation Coma Berenices. NGC 4070 was discovered by astronomer William Herschel on April 27, 1785. It was rediscovered by John Herschel on April 29, 1832 and was listed as NGC 4059. The galaxy is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4074</span> Galaxy in the constellation Coma Berenices

NGC 4074 is a peculiar lenticular galaxy located 310 million light-years away in the constellation Coma Berenices. It 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 4076</span> Spiral 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 4306</span> Dwarf barred lenticular galaxy in the constellation Virgo

NGC 4306 is a dwarf barred lenticular galaxy located about 100 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer Heinrich d'Arrest on April 16, 1865. Although considered to be a member of the Virgo Cluster, its high radial velocity and similar distance as NGC 4305 suggest that NGC 4306 is a background galaxy. NGC 4306 is a companion of NGC 4305 and appears to be interacting with it.

<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.

<span class="mw-page-title-main">NGC 4393</span> Spiral 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 "NASA/IPAC Extragalactic Database". Results for NGC 4709. Retrieved 2018-04-12.
  2. 1 2 New horizons in globular cluster astronomy : proceedings of a conference held at Università di Padova, Padova, Italy, 24-28 June, 2002. King, Ivan R., Piotto, G. (Giampaolo) (1st ed.). San Francisco, Calif.: Astronomical Society of the Pacific. 2003. ISBN   978-1583811436. OCLC   54022703.{{cite book}}: CS1 maint: others (link)
  3. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-04-13.
  4. ↑ "Revised NGC Data for NGC 4709". spider.seds.org. Retrieved 2018-04-13.
  5. ↑ Jerjen, H.; Dressler, A. (1997-07-01). "Studies of the Centaurus cluster". Astronomy and Astrophysics Supplement Series. 124 (1): 1–12. Bibcode:1997A&AS..124....1J. doi: 10.1051/aas:1997355 . ISSN   0365-0138.
  6. ↑ O'Meara, Stephen James (2013-04-08). Deep-Sky Companions: Southern Gems. Cambridge University Press. p. 460. Bibcode:2013dcsg.book.....O. ISBN   978-1-139-85154-1.
  7. ↑ Lucey, J. R.; Currie, Malcom J.; Dickens, R. J. (1986-07-01). "The Centaurus cluster of galaxies – II. The bimodal velocity structure". Monthly Notices of the Royal Astronomical Society. 221 (2): 453–472. Bibcode:1986MNRAS.221..453L. doi: 10.1093/mnras/221.2.453 . ISSN   0035-8711.
  8. 1 2 Churazov, E.; Gilfanov, M.; Forman, W.; Jones, C. (1999). "Evidence for Merging in the Centaurus Cluster". The Astrophysical Journal. 520 (1): 105. arXiv: astro-ph/9802166 . Bibcode:1999ApJ...520..105C. doi:10.1086/307421. ISSN   0004-637X. S2CID   18552647.
  9. ↑ Walker, S. A.; Fabian, A. C.; Sanders, J. S. (2013-11-11). "An XMM–Newton view of the merging activity in the Centaurus cluster". Monthly Notices of the Royal Astronomical Society. 435 (4): 3221–3230. arXiv: 1308.2090 . Bibcode:2013MNRAS.435.3221W. doi:10.1093/mnras/stt1515. ISSN   0035-8711.
  10. ↑ "New General Catalog Objects: NGC 4700 - 4749". cseligman.com. Retrieved 2018-04-11.
  11. ↑ Lucey, J. R.; Currie, Malcolm J.; Dickens, R. J. (1986-10-01). "The Centaurus cluster of galaxies – III. Its structure and the distribution of the different galaxy types". Monthly Notices of the Royal Astronomical Society. 222 (3): 427–447. Bibcode:1986MNRAS.222..427L. doi: 10.1093/mnras/222.3.427 . ISSN   0035-8711.


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