Astronomy:NGC 4939

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Short description: Spiral galaxy in the constellation Virgo
NGC 4939
Ngc4939-hst-606.png
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension 13h 04m 14.4s[1]
Declination−10° 20′ 22″[1]
Redshift0.010374 ± 0.000013 [1]
Helio radial velocity3,110 ± 4 km/s[1]
Distance118 ± 30 Mly (36.1 ± 9.4 Mpc)[1]
Apparent magnitude (V)11.3[2]
Characteristics
TypeSA(s)bc [1]
Apparent size (V)5.5′ × 2.8′[1]
Notable featuresSeyfert galaxy
Other designations
MCG -02-33-104, PGC 45170[1]

NGC 4939 is a spiral galaxy located in the constellation Virgo. It is located at a distance of about 120 million light years from Earth, which, given its apparent dimensions, means that NGC 4939 is about 190,000 light years across. It was discovered by William Herschel on March 25, 1786.[3]

Characteristics

NGC 4939 has been characterised as a Seyfert galaxy, a galaxy category which features bright point-like nuclei. NGC 4939 is a type II Seyfert galaxy. Its X-ray spectrum is more consistent with a Compton-thick cold reflection source, which means that the source is hidden behind dense material, mainly gas and dust, and the X-rays observed have been reflected, but a Compton-thin transmission model could not be ruled out.[4] The equivalent width of the FeKα line is large, indicating too that it is a Compton-thick source.[5] Further observations by Swift Observatory confirmed its Compton-thick nature.[6] The source of activity in the active galactic nuclei is a supermassive black hole (SMBH) lying at the centre of the galaxy. The SMBH at the centre of NGC 4939 is accreting material with a rate of 0.077 M☉ per year.[7] The black hole has been detected in hard X-rays, which are not absorbed by the Compton-thick column, by INTEGRAL.[8]

The galaxy has a large elliptical bulge and maybe a weak bar. It is a grand design spiral galaxy, with two tightly wrapped arms emanating from the bulge. The arms are thin, smooth and well defined and can be traced for nearly one and a half revolutions before fading.[9] Two symmetric arm sections or arcs are observed in the central part of the galaxy.[10] The galaxy is seen with an inclination of 56 degrees. The rotational speed of the galaxy is about 270 km/s.[11]

Supernovae

NGC 4939 has been home of five supernovae: SN 1968X (mag. 16),[12] SN 1973J (mag. 16),[13] SN 2008aw (Type II, mag. 15.9),[14] SN 2014B (Type IIP, mag. 17.0),[15] and SN 2020nif (Type II, mag. 16.1).[16]

Nearby galaxies

NGC 4939 belongs to a small galaxy group known as the NGC 4933 group, named after the multiple galaxy NGC 4933.[17] The group lies between the Local Supercluster and Hydra-Centaurus Supercluster.[18]

References

  1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 "NASA/IPAC Extragalactic Database". Results for NGC 4939. http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=NGC+4939. 
  2. ↑ "Revised NGC Data for NGC 4939". http://spider.seds.org/ngc/revngcic.cgi?NGC4939. 
  3. ↑ Seligman, Courtney. "NGC 4939 (= PGC 45170)". http://cseligman.com/text/atlas/ngc49.htm#4939. 
  4. ↑ Maiolino, R.; Salvati, M.; Bassani, L.; Dadina, M.; della Ceca, R.; Matt, G.; Risaliti, G.; Zamorani, G. (October 1998). "Heavy obscuration in X-ray weak AGNs". Astronomy and Astrophysics 338: 781–794. Bibcode: 1998A&A...338..781M. 
  5. ↑ Dadina, M. (4 October 2006). "BeppoSAX observations in the 2–100 keV band of the nearby Seyfert galaxies: an atlas of spectra". Astronomy & Astrophysics 461 (3): 1209–1252. doi:10.1051/0004-6361:20065734. 
  6. ↑ Vasudevan, Ranjan V.; Brandt, William N.; Mushotzky, Richard F.; Winter, Lisa M.; Baumgartner, Wayne H.; Shimizu, Thomas T.; Schneider, Donald. P.; Nousek, John (15 January 2013). "X-ray properties of the northern galactic cap sources in the 58 month Swift/BAT catalog". The Astrophysical Journal 763 (2): 111. doi:10.1088/0004-637X/763/2/111. Bibcode: 2013ApJ...763..111V. 
  7. ↑ Diamond-Stanic, Aleksandar M.; Rieke, George H. (20 February 2012). "The relationship between black hole growth and star formation in Seyfert galaxies". The Astrophysical Journal 746 (2): 168. doi:10.1088/0004-637X/746/2/168. Bibcode: 2012ApJ...746..168D. 
  8. ↑ "IGR J13042-1020: a massive black hole in spiral galaxy NGC 4939". ESA. 11 June 2010. http://sci.esa.int/integral/47176-igr-j13042-1020-a-massive-black-hole-in-ngc-4939/. 
  9. ↑ Eskridge, Paul B.; Frogel, Jay A.; Pogge, Richard W.; Quillen, Alice C.; Berlind, Andreas A.; Davies, Roger L.; DePoy, D. L.; Gilbert, Karoline M. et al. (November 2002). "Near-Infrared and Optical Morphology of Spiral Galaxies". The Astrophysical Journal Supplement Series 143 (1): 73–111. doi:10.1086/342340. Bibcode: 2002ApJS..143...73E. 
  10. ↑ Grosbøl, P.; Patsis, P. A.; Pompei, E. (12 August 2004). "Spiral galaxies observed in the near-infrared K band". Astronomy & Astrophysics 423 (3): 849–859. doi:10.1051/0004-6361:20035804. 
  11. ↑ Mitchell, Carl J.; Sellwood, J. A.; Williams, T. B.; Spekkens, Kristine; Kuzio de Naray, Rachel; Bixel, Alex (23 February 2018). "The RINGS Survey. III. Medium-resolution H-alpha Fabry–Pérot Kinematic Data Set". The Astronomical Journal 155 (3): 123. doi:10.3847/1538-3881/aaabb8. Bibcode: 2018AJ....155..123M. 
  12. ↑ Transient Name Server entry for SN 1968X. Retrieved 24 March 2023.
  13. ↑ Transient Name Server entry for SN 1973J. Retrieved 24 March 2023.
  14. ↑ Transient Name Server entry for SN 2008aw. Retrieved 24 March 2023.
  15. ↑ Transient Name Server entry for SN 2014B. Retrieved 24 March 2023.
  16. ↑ Transient Name Server entry for SN 2020nif. Retrieved 24 March 2023.
  17. ↑ 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. doi:10.1111/j.1365-2966.2010.18071.x. Bibcode: 2011MNRAS.412.2498M. http://www.sao.ru/hq/dim/groups/galaxies.dat. Retrieved 18 December 2018. 
  18. ↑ Richter, O. -G.; Huchtmeier, W. K. (1 March 1987). "HI observations of galaxies in between the Local and the Hydra/Centaurus superclusters.". Astronomy and Astrophysics Supplement Series 68: 427–467. ISSN 0365-0138. Bibcode: 1987A&AS...68..427R. https://ui.adsabs.harvard.edu/abs/1987A%26AS...68..427R/abstract. 

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