NGC 3860

Last updated
NGC 3860
NGC 3860 legacy dr10.jpg
legacy surveys image of NGC 3860 (upper right) and NGC 3860B (lower left).
Observation data (J2000 epoch)
Constellation Leo
Right ascension 11h 44m 49.1s [1]
Declination 19° 47′ 42″ [1]
Redshift 0.018663 [1]
Helio radial velocity 5595 km/s [1]
Distance 340  Mly (105  Mpc) [1]
Group or cluster Leo Cluster
Apparent magnitude  (V)14.22 [1]
Characteristics
Type Sa [1]
Mass ~3.7×1011 [2]   M☉
Size~133,000  ly (40.7  kpc) (estimated) [1]
Apparent size  (V)1.0 x 0.5 [1]
Other designations
CGCG 97-120, IRAS 11422+2003, MCG 3-30-88, PGC 36577, UGC 6718 [1]

NGC 3860 is a spiral galaxy [3] located about 340 million light-years away [4] in the constellation Leo. [5] NGC 3860 was discovered by astronomer William Herschel on April 27, 1785. [6] The galaxy is a member of the Leo Cluster [7] [8] and is a low-luminosity AGN (LLAGN). [9] [10] 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. [11]

Contents

H I deficiency

Observations of NGC 3860 show that the galaxy has lost approximately 90% of its original hydrogen content. This indicates that NGC 3860 has crossed though the core of the Leo Cluster and that ram pressure exerted by the dense intergalactic medium in the cluster stripped most of the neutral atomic hydrogen from the galaxy. [12]

The gas disk of NGC 3860 is truncated, which is an additional indicator that the galaxy is undergoing ram pressure stripping as it falls into the Leo Cluster. [13]

See also

Related Research Articles

<span class="mw-page-title-main">NGC 4309</span> 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.

<span class="mw-page-title-main">NGC 3862</span> Galaxy in the constellation Leo

NGC 3862 is an elliptical galaxy located 300 million light-years away in the constellation Leo. Discovered by astronomer William Herschel on April 27, 1785, NGC 3862 is an outlying member of the Leo Cluster.

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

The Coma I Group is a group of galaxies located about 14.5 Mpc (47.3 Mly) away in the constellation Coma Berenices. The brightest member of the group is NGC 4725. The Coma I Group is rich in spiral galaxies while containing few elliptical and lenticular galaxies. Coma I lies in the foreground of the more distant Coma and Leo clusters and is located within the Virgo Supercluster.

<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 3844</span> Galaxy in the constellation Leo

NGC 3844 is a lenticular 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 3844 is a member of the Leo Cluster and is likely to be a low-luminosity AGN (LLAGN).

<span class="mw-page-title-main">NGC 3845</span> Galaxy in the constellation Leo

NGC 3845 is a barred lenticular galaxy located about 270 million light-years away in the constellation Leo. NGC 3845 was discovered by astronomer John Herschel on March 17, 1831. It is a member of the Leo Cluster and is likely to be a low-luminosity AGN (LLAGN).

<span class="mw-page-title-main">NGC 3861</span> Galaxy in the constellation Leo

NGC 3861 is a large barred spiral galaxy with a ring-like structure located about 310 million light-years away in the constellation Leo. It was discovered by astronomer John Herschel on March 23, 1827. NGC 3861 is a member of the Leo Cluster and has a normal amount of neutral hydrogen and ionised hydrogen.

<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 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 4061</span> Galaxy in the constellation Coma Berenices

NGC 4061 is an elliptical galaxy located 310 light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 27, 1785. It was rediscovered by John Herschel on April 29, 1832. It is listed both as NGC 4061 and NGC 4055. NGC 4061 is a member of the NGC 4065 Group and forms an interacting pair with its companion, NGC 4065 as evidenced by distortions in their optical isophotes.

<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 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> 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 4089</span> Galaxy in the constellation of Coma Berenices

NGC 4089 is an elliptical galaxy located 340 million light-years away in the constellation Coma Berenices. NGC 4089 was discovered by astronomer Heinrich d'Arrest on May 4, 1864 and is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4090</span> Galaxy in the constellation Coma Berenices

NGC 4090 is a spiral galaxy located 340 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer Heinrich d'Arrest on May 2, 1864 and is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4092</span> Galaxy in the constellation Coma Berenices

NGC 4092 is a spiral galaxy located 310 million light-years away in the constellation Coma Berenices. It was discovered by astronomer Heinrich d'Arrest on May 2, 1864. NGC 4092 is a member of the NGC 4065 Group and hosts an AGN.

<span class="mw-page-title-main">NGC 4095</span> Galaxy in the constellation Coma Berenices

NGC 4095 is an elliptical galaxy located 330 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 26, 1785. NGC 4095 is a member of the NGC 4065 Group and is a LINER.

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

The NGC 4065 Group is a group of galaxies located about 330 Mly (100 Mpc) in the constellation Coma Berenices. The group's brightest member is NGC 4065 and located in the Coma Supercluster.

<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 10 "NASA/IPAC Extragalactic Database". Results for NGC 3860. Retrieved 2018-07-23.
  2. ↑ Sun, M.; Murray, S. S. (2002). "Chandra View of the Dynamically Young Cluster of Galaxies A1367. I. Small-Scale Structures". The Astrophysical Journal. 576 (2): 708. arXiv: astro-ph/0206255 . Bibcode:2002ApJ...576..708S. doi:10.1086/341756. ISSN   0004-637X. S2CID   11414230.
  3. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-07-23.
  4. ↑ "NED Query Results for NGC 3860". ned.ipac.caltech.edu. Retrieved 2018-07-23.
  5. ↑ "Revised NGC Data for NGC 3860". spider.seds.org. Retrieved 2018-07-23.
  6. ↑ "New General Catalog Objects: NGC 3850 - 3899". cseligman.com. Retrieved 2018-07-17.
  7. ↑ "NGC 3860" . Retrieved 2018-07-24.
  8. ↑ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-07-24.
  9. ↑ Sun, M.; Murray, S. S. (2002). "Chandra View of the Dynamically Young Cluster of Galaxies A1367. II. Point Sources". The Astrophysical Journal. 577 (1): 139–149. arXiv: astro-ph/0202431 . Bibcode:2002ApJ...577..139S. doi:10.1086/342156. ISSN   0004-637X. S2CID   119421982.
  10. ↑ Caglar, Turgay; Hudaverdi, Murat (2017-08-31). "XMM–Newton view of X-ray overdensities from nearby galaxy clusters: the environmental dependencies". Monthly Notices of the Royal Astronomical Society. 471 (4): 4990–5007. arXiv: 1709.00117 . Bibcode:2017MNRAS.471.4990C. doi:10.1093/mnras/stx1811. ISSN   0035-8711. S2CID   39126208.
  11. ↑ Gavazzi, G.; Savorgnan, G.; Fumagalli, Mattia (2011-09-26). "The complete census of optically selected AGNs in the Coma supercluster: the dependence of AGN activity on the local environment". Astronomy & Astrophysics. 534: A31. arXiv: 1107.3702 . Bibcode:2011A&A...534A..31G. doi:10.1051/0004-6361/201117461. ISSN   0004-6361. S2CID   73621726.
  12. ↑ Gavazzi, G.; Cortese, L.; Boselli, A.; Iglesias-Paramo, J.; Vílchez, J. M.; Carrasco, L. (2003). "Capturing a Star Formation Burst in Galaxies Infalling onto the Cluster A1367". The Astrophysical Journal. 597 (1): 210–217. arXiv: astro-ph/0307075 . Bibcode:2003ApJ...597..210G. doi:10.1086/378264. ISSN   0004-637X. S2CID   119076926.
  13. ↑ Fossati, Matteo; Fumagalli, Michele; Gavazzi, Giuseppe; Consolandi, Guido; Boselli, Alessandro; Yagi, Masafumi; Sun, Ming; Wilman, David J. (2019-04-01). "MUSE sneaks a peek at extreme ram-pressure stripping events - IV. Hydrodynamic and gravitational interactions in the Blue Infalling Group". Monthly Notices of the Royal Astronomical Society. 484 (2): 2212–2228. arXiv: 1901.03334 . Bibcode:2019MNRAS.484.2212F. doi:10.1093/mnras/stz136. ISSN   0035-8711. S2CID   118857397.


This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.