NGC 5363

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NGC 5363
NGC5363 - SDSS DR14.jpg
NGC 5363 by SDSS
Observation data (J2000 epoch)
Constellation Virgo
Right ascension 13h 56m 07.2s [1]
Declination +05° 15′ 17″ [1]
Redshift 0.003799 ± 0.000017 [1]
Helio radial velocity 1,139 ± 5 km/s [1]
Distance 63.6 ± 13 Mly (19.5 ± 4.1 Mpc) [1]
Apparent magnitude  (V)10.5 [2]
Characteristics
Type I0? [1] /S0 [3]
Apparent size  (V)4.1′ × 2.6′ [1]
Notable features LINER, spiral dust disk
Other designations
UGC 8847, CGCG 046-007, MCG +01-36-002, PGC 49547 [1]

NGC 5363 is a lenticular galaxy located in the constellation Virgo. It is located at a distance of circa 65 million light years from Earth, which, given its apparent dimensions, means that NGC 5363 is about 100,000 light years across. It was discovered by William Herschel on January 19, 1784. [4] It is a member of the NGC 5364 Group of galaxies, itself one of the Virgo III Groups strung out to the east of the Virgo Supercluster of galaxies. [5]

Contents

Characteristics

NGC 5363 is characterised by the presence of a dust lane along its minor axis, visible also in mid-infrared maps, [6] and a more extended one with an intermediate orientation. [7] The total mass of cold dust in the galaxy is estimated to be 2×106 M☉, extending for 52 arcseconds in the far-infrared. [8] The dust emission appears as a disk with spiral arms and a possible barlike structure, and extends at the outer parts of the galaxy as a fainter, armlike structure, along the major axis of the galaxy. [9] The galaxy also features HII emission that forms a spiral disk. [10]

The total dust mass is about a factor of 100 larger than the one predicted if it was created only by the mass lost by evolved stars. [7] The galaxy also has shells, which are evidence of a recent merger, in which NGC 5363 accreted another galaxy, and thus it is strongly suggested that the interstellar dust is of external origin. [10] It is highly likely that this merger event caused star formation activity in the galaxy, as is evident by the detection of ultraviolet radiation associated with young stars. [10]

Based on its spectrum, the nucleus of NGC 5363 has been found to be active and has been categorised as a LINER. [11] In the centre of NGC 5363 lies a supermassive black hole with an estimated mass of 375 million M☉. [12] NGC 5363 has been found to emit radio waves. The radio source consists of a compact core with a diameter of less than 2 arcseconds and probably an extended component, stretching for about 20 arcseconds. [13]

Nearby galaxies

NGC 5363 is the foremost galaxy in a galaxy group known as the NGC 5363 group. Other members of the group include NGC 5300, NGC 5348, NGC 5356, NGC 5360, and NGC 5364. [14] NGC 5363 and NGC 5364 lie at a projected distance of 14.5 arcminutes, forming a non-interacting pair. [15] The group is part of the Virgo III Groups, a very obvious chain of galaxy groups on the left side of the Virgo cluster, stretching across 40 million light years of space. [16]

See also

Related Research Articles

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<span class="mw-page-title-main">NGC 2336</span> Galaxy in the constellation Camelopardalis

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<span class="mw-page-title-main">NGC 3367</span> Spiral galaxy in the constellation Leo

NGC 3367 is a barred spiral galaxy located in the constellation Leo. It is located at a distance of about 120 million light years from Earth, which, given its apparent dimensions, means that NGC 3367 is about 85,000 light years across. It was discovered by William Herschel on March 19, 1784.

<span class="mw-page-title-main">NGC 7130</span> Galaxy in the constellation Piscis Austrinus

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<span class="mw-page-title-main">NGC 5982</span> Galaxy in the constellation Draco

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<span class="mw-page-title-main">NGC 3489</span> Galaxy in the constellation Leo

NGC 3489 is a lenticular galaxy located in the constellation Leo. It is located at a distance of circa 30 million light years from Earth, which, given its apparent dimensions, means that NGC 3489 is about 30,000 light years across. It was discovered by William Herschel on April 8, 1784. NGC 3489 is a member of the Leo Group.

<span class="mw-page-title-main">NGC 4636</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 5846</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 1386</span> Galaxy in the constellation Eridanus

NGC 1386 is a spiral galaxy located in the constellation Eridanus. It is located at a distance of circa 53 million light years from Earth, which, given its apparent dimensions, means that NGC 1386 is about 50,000 light years across. It is a Seyfert galaxy, the only one in Fornax Cluster.

<span class="mw-page-title-main">NGC 4278</span> Galaxy in the constellation Coma Berenices

NGC 4278 is an elliptical galaxy located in the constellation Coma Berenices. It is located at a distance of circa 55 million light years from Earth, which, given its apparent dimensions, means that NGC 4278 is about 65,000 light years across. It was discovered by William Herschel on March 13, 1785. NGC 4278 is part of the Herschel 400 Catalogue and can be found about one and 3/4 of a degree northwest of Gamma Comae Berenices even with a small telescope.

<span class="mw-page-title-main">NGC 7418</span> Galaxy in the constellation Grus

NGC 7418 is an intermediate spiral galaxy located in the constellation Grus. It is located at a distance of circa 60 million light-years from Earth, which, given its apparent dimensions, means that NGC 7418 is about 60,000 light-years across. It was discovered by John Herschel on August 30, 1834.

<span class="mw-page-title-main">NGC 2273</span> Galaxy in the constellation Lynx

NGC 2273 is a barred spiral galaxy located in the constellation Lynx. It is located at a distance of circa 95 million light years from Earth, which, given its apparent dimensions, means that NGC 2273 is about 100,000 light years across. It was discovered by Nils Dunér on September 15, 1867.

References

  1. 1 2 3 4 5 6 7 8 "NASA/IPAC Extragalactic Database". Results for NGC 5363. Retrieved 2016-01-18.
  2. ↑ "Revised NGC Data for NGC 5363". spider.seds.org. Retrieved 25 November 2018.
  3. ↑ Ho, L. C.; Filippenko, A. V.; Sargent, W. L. (June 1995). "A search for 'dwarf' Seyfert nuclei. 2: an optical spectral atlas of the nuclei of nearby galaxies". The Astrophysical Journal Supplement Series. 98: 477. Bibcode:1995ApJS...98..477H. doi: 10.1086/192170 .
  4. ↑ Seligman, Courtney. "NGC 5363 (= PGC 49547)". Celestial Atlas. Retrieved 19 November 2018.
  5. ↑ "The Virgo III Groups". Atlas of the Universe. Retrieved 2010-11-27.
  6. ↑ Xilouris, E. M.; Madden, S. C.; Galliano, F.; Vigroux, L.; Sauvage, M. (26 February 2004). "Dust emission in early-type galaxies: The mid-infrared view". Astronomy & Astrophysics. 416 (1): 41–55. arXiv: astro-ph/0312029 . Bibcode:2004A&A...416...41X. doi:10.1051/0004-6361:20034020. S2CID   12635736.
  7. 1 2 Patil, M. K.; Pandey, S. K.; Sahu, D. K.; Kembhavi, A. (26 September 2006). "Properties of dust in early-type galaxies". Astronomy & Astrophysics. 461 (1): 103–113. arXiv: astro-ph/0611369 . doi:10.1051/0004-6361:20053512. S2CID   119476971.
  8. ↑ Temi, Pasquale; Brighenti, Fabrizio; Mathews, William G.; Bregman, Jesse D. (April 2004). "Cold Dust in Early-Type Galaxies. I. Observations". The Astrophysical Journal Supplement Series. 151 (2): 237–269. arXiv: astro-ph/0312248 . Bibcode:2004ApJS..151..237T. doi:10.1086/381963. S2CID   118856747.
  9. ↑ Pahre, Michael A.; Ashby, M. L. N.; Fazio, G. G.; Willner, S. P. (September 2004). "Spatial Distribution of Warm Dust in Early-Type Galaxies". The Astrophysical Journal Supplement Series. 154 (1): 229–234. arXiv: astro-ph/0406379 . Bibcode:2004ApJS..154..229P. doi:10.1086/423320. S2CID   8841216.
  10. 1 2 3 Finkelman, Ido; Brosch, Noah; Funes, José G.; Kniazev, Alexei Y.; Väisänen, Petri (22 July 2010). "Ionized gas in E/S0 galaxies with dust lanes". Monthly Notices of the Royal Astronomical Society. 407 (4): 2475–2500. arXiv: 1005.4227 . Bibcode:2010MNRAS.407.2475F. doi:10.1111/j.1365-2966.2010.17070.x. S2CID   117552408.
  11. ↑ Ho, Luis C.; Filippenko, Alexei V.; Sargent, Wallace L. W. (October 1997). "A Search for "Dwarf Seyfert Nuclei. III. Spectroscopic Parameters and Properties of the Host Galaxies". The Astrophysical Journal Supplement Series. 112 (2): 315–390. arXiv: astro-ph/9704107 . Bibcode:1997ApJS..112..315H. doi:10.1086/313041. S2CID   17086638.
  12. ↑ Saikia, Payaswini; Körding, Elmar; Falcke, Heino (July 2015). "The Fundamental Plane of black hole activity in the optical band". Monthly Notices of the Royal Astronomical Society. 450 (3): 2317–2326. arXiv: 1504.00363 . Bibcode:2015MNRAS.450.2317S. doi:10.1093/mnras/stv731. S2CID   118515692.
  13. ↑ Tovmasian, G. M.; Sramek, R. A. (November 1976). "The radio emission of NGC 5363". Astrofizika. 12: 693–696. Bibcode:1976Afz....12..693T.
  14. ↑ Makarov, Dmitry; Karachentsev, Igor (21 April 2011). "Galaxy groups and clouds in the local (z~ 0.01) Universe". Monthly Notices of the Royal Astronomical Society. 412 (4): 2498–2520. arXiv: 1011.6277 . Bibcode:2011MNRAS.412.2498M. doi:10.1111/j.1365-2966.2010.18071.x. S2CID   119194025. Archived from the original on 31 January 2016. Retrieved 4 February 2019.
  15. ↑ de Vaucouleurs, G.; de Vaucouleurs, A.; Corwin, J. R. (1976). "Second reference catalogue of bright galaxies". Second Reference Catalogue of Bright Galaxies. 1976. Bibcode:1976RC2...C......0D.
  16. ↑ "The Virgo III Groups". www.atlasoftheuniverse.com. Retrieved 9 January 2019.


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