NGC 4939

Last updated • 2 min readFrom Wikipedia, The Free Encyclopedia
NGC 4939
Ngc4939-hst-606.png
NGC 4939 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
Constellation Virgo
Right ascension 13h 04m 14.3133s [1]
Declination −10° 20′ 22.417″ [1]
Redshift 0.010561 [1]
Heliocentric radial velocity 3166 ± 2 km/s [1]
Distance 118 ± 30 Mly (36.1 ± 9.4 Mpc) [1]
Apparent magnitude  (V)11.3 [2]
Characteristics
Type SA(s)bc [1]
Size~192,800  ly (59.10  kpc) (estimated) [1]
Apparent size  (V)5.5′ × 2.8′ [1]
Notable featuresSeyfert galaxy
Other designations
IRAS 13016-1004, MCG -02-33-104, PGC 45170 [1]

NGC 4939 is a large 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]

Contents

Characteristics

NGC 4939 imaged by Adam Block in 2014. Noao-n4939block.jpg
NGC 4939 imaged by Adam Block in 2014.

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

Five supernovae have been observed in NGC 4939:

Nearby galaxies

NGC 4939 belongs to a small galaxy group known as the NGC 4933 group, named after the multiple galaxy NGC 4933. [20] The group lies between the Local Supercluster and Hydra-Centaurus Supercluster. [21]

References

  1. 1 2 3 4 5 6 7 8 9 "Results for object NGC 4939". NASA/IPAC Extragalactic Database. NASA and Caltech . Retrieved 2016-01-18.
  2. ↑ "Revised NGC Data for NGC 4939". spider.seds.org. Retrieved 25 November 2018.
  3. ↑ Seligman, Courtney. "NGC 4939 (= PGC 45170)". Celestial Atlas. Retrieved 19 November 2018.
  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. arXiv: astro-ph/9806055 . 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. Bibcode:2007A&A...461.1209D. 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. arXiv: 1212.2957 . Bibcode:2013ApJ...763..111V. doi:10.1088/0004-637X/763/2/111. S2CID   118854864.
  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. arXiv: 1106.3565 . Bibcode:2012ApJ...746..168D. doi:10.1088/0004-637X/746/2/168. S2CID   119277531.
  8. ↑ "IGR J13042-1020: a massive black hole in spiral galaxy NGC 4939". sci.esa.int. ESA. 11 June 2010.
  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.; Houdashelt, Mark L.; Kuchinski, Leslie E.; Ramirez, Solange V.; Sellgren, K.; Stutz, Amelia; Terndrup, Donald M.; Tiede, Glenn P. (November 2002). "Near-Infrared and Optical Morphology of Spiral Galaxies". The Astrophysical Journal Supplement Series. 143 (1): 73–111. arXiv: astro-ph/0206320 . Bibcode:2002ApJS..143...73E. doi:10.1086/342340. S2CID   15491635.
  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. arXiv: 1801.07750 . Bibcode:2018AJ....155..123M. doi: 10.3847/1538-3881/aaabb8 . S2CID   59472535.
  12. ↑ Marsden, Brian G. (3 December 1968). "Circular No. 2116". Central Bureau for Astronomical Telegrams. Smithsonian Astrophysical Observatory, IAU . Retrieved 22 December 2024.
  13. ↑ "SN 1968X". Transient Name Server. IAU . Retrieved 22 December 2024.
  14. ↑ "SN 1973J". Transient Name Server. IAU . Retrieved 22 December 2024.
  15. ↑ Winslow, D.; Li, W.; Filippenko, A. V. (2008). "Supernova 2008aw in NGC 4939". Central Bureau Electronic Telegrams (1279): 1. Bibcode:2008CBET.1279....1W.
  16. ↑ "SN 2008aw". Transient Name Server. IAU . Retrieved 22 December 2024.
  17. ↑ Kim, H.; Zheng, W.; Li, W.; Filippenko, A. V.; Cenko, S. B. (2014). "Supernova 2014B in NGC 4939 = PSN J13041770-1020012". Central Bureau Electronic Telegrams (3772): 1. Bibcode:2014CBET.3772....1K.
  18. ↑ "SN 2014B". Transient Name Server. IAU . Retrieved 22 December 2024.
  19. ↑ "SN 2020nif". Transient Name Server. IAU . Retrieved 22 December 2024.
  20. ↑ 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.
  21. ↑ 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. Bibcode:1987A&AS...68..427R. ISSN   0365-0138.
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.