NGC 3631

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NGC 3631
Hubble Looks at a Face-On Grand Spiral.jpg
NGC 3631 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
Constellation Ursa Major
Right ascension 11h 21m 02.8753s [1]
Declination +53° 10′ 11.038″ [1]
Redshift 0.003839 [1]
Heliocentric radial velocity 1151 ± 1 km/s [1]
Distance 33.7 ± 17.7 Mly (10.3 ± 5.4 Mpc) [1]
Group or cluster NGC 3631 Group (LGG 241)
Apparent magnitude  (V)10.1
Characteristics
Type SA(s)c [1]
Size~56,700  ly (17.39  kpc) (estimated) [1]
Apparent size  (V)5.0′ × 4.8′ [1]
Other designations
Arp 27, UGC 6360, MCG +09-19-047, PGC 34767, VV 363 [1]

NGC 3631 is a spiral galaxy located in the constellation Ursa Major. It is located at a distance of about 35 million light years from Earth, which, given its apparent dimensions, means that NGC 3631 is about 60,000 light years across. It was discovered by William Herschel on April 14, 1789. [2] It is a grand design spiral galaxy seen face on.

Contents

Characteristics

NGC 3631 is a grand design spiral galaxy and features two principal spiral arms, which begin near the center. The two main arms branch into secondary arms with lower surface brightness. The galaxy shows moderate-to-high star formation rate and bright HII regions are present in all the arms. [3] The star formation rate of the galaxy is 4.6 M☉ per year. [4] Halton Arp observed "straight arms", and an "absorption tube crossing from inside to outside of southern arm" and added the galaxy to his Atlas of Peculiar Galaxies. [5] At inclination of 17 degrees, [5] the galaxy is seen nearly face on.

The HI imaging shows the spiral arms distinguished well and HI is also detected in most of the interarm regions. The atomic hydrogen is detected mostly within the limits of the optical disc but also extends one and a half times the radius of the optical disk. The hydrogen forms streaming motions near the spiral arms. [6] The gas features two anticyclonic and four cyclonic vortices, rotating with the spiral pattern. The anticyclones are caused by the differential rotation and the cyclones are the result of a high amplitude in the density wave. The centres of the anticyclones are located between the observed spiral arms and the cyclones lie close to the observed spirals. [5]

NGC 3631 has weak diffuse X-ray emission. [7] There are six candidates ultraluminous X-ray sources in disk of the galaxy, two which have an optical counterpart. [8] The nucleus of the galaxy hosts a supermassive black hole with mass 107.4 (25 million) M☉, based on Ks bulge luminosity. [9]

Supernovae

Four supernovae have been discovered in NGC 3631:

Nearby galaxies and group

NGC 3631 forms a small group with NGC 3657, [18] which is part of the north Ursa Major groups, [19] which is part of the Ursa Major Cloud, [20] [21] which is part of the Virgo Supercluster. [19]

According to A.M. Garcia, NGC 3631 is part of the NGC 3631 galaxy group (also known as LGG 241). This group includes at least 10 galaxies, including NGC 3657, NGC 3718, NGC 3729, NGC 3913, NGC 3972, NGC 3998, UGC 6251, UGC 6446, and UGC 6816. [22]

References

  1. 1 2 3 4 5 6 7 8 9 "NASA/IPAC Extragalactic Database". Results for NGC 3631. Retrieved 2016-01-18.
  2. ↑ NGC 3631 cseligman.com
  3. ↑ Sandage, A., Bedke, J. (1994) The Carnegie Atlas of Galaxies. Volume I, Carnegie Institution of Washington
  4. ↑ Mineo, S.; Gilfanov, M.; Lehmer, B. D.; Morrison, G. E.; Sunyaev, R. (11 January 2014). "X-ray emission from star-forming galaxies – III. Calibration of the LX-SFR relation up to redshift z ≈ 1.3". Monthly Notices of the Royal Astronomical Society. 437 (2): 1698–1707. arXiv: 1207.2157 . Bibcode:2014MNRAS.437.1698M. doi: 10.1093/mnras/stt1999 . S2CID   119190124.
  5. 1 2 3 Fridman, A. M.; Khoruzhii, O. V.; Polyachenko, E. V.; Zasov, A. V.; Sil'Chenko, O. K.; Moiseev, A. V.; Burlak, A. N.; Afanasiev, V. L.; Dodonov, S. N.; Knapen, J. H. (21 May 2001). "Gas motions in the plane of the spiral galaxy NGC 3631". Monthly Notices of the Royal Astronomical Society. 323 (3): 651–662. arXiv: astro-ph/0012116 . Bibcode:2001MNRAS.323..651F. doi: 10.1046/j.1365-8711.2001.04218.x . S2CID   119517678.
  6. ↑ Knapen, J. H. (1 April 1997). "Atomic hydrogen in the spiral galaxy NGC 3631". Monthly Notices of the Royal Astronomical Society. 286 (2): 403–414. arXiv: astro-ph/9612137 . Bibcode:1997MNRAS.286..403K. doi: 10.1093/mnras/286.2.403 . S2CID   13901223.
  7. ↑ Mineo, S.; Gilfanov, M.; Sunyaev, R. (1 November 2012). "X-ray emission from star-forming galaxies - II. Hot interstellar medium". Monthly Notices of the Royal Astronomical Society. 426 (3): 1870–1883. arXiv: 1205.3715 . Bibcode:2012MNRAS.426.1870M. doi: 10.1111/j.1365-2966.2012.21831.x . S2CID   85507925.
  8. ↑ Smith, Beverly J.; Swartz, Douglas A.; Miller, Olivia; Burleson, Jacob A.; Nowak, Michael A.; Struck, Curtis (1 June 2012). "ChAInGeS: The Chandra Arp Interacting Galaxies Survey". The Astronomical Journal. 143 (6): 144. arXiv: 1204.3194 . Bibcode:2012AJ....143..144S. doi:10.1088/0004-6256/143/6/144. S2CID   17427760.
  9. ↑ Dong, X. Y.; De Robertis, M. M. (March 2006). "Low-Luminosity Active Galaxies and Their Central Black Holes". The Astronomical Journal. 131 (3): 1236–1252. arXiv: astro-ph/0510694 . Bibcode:2006AJ....131.1236D. doi:10.1086/499334. S2CID   17630682.
  10. ↑ "SN 1964A". Transient Name Server. IAU . Retrieved 1 December 2024.
  11. ↑ Wild, P.; Rosino, L.; Zwicky, F. (1965). "Supernova in NGC 3631". International Astronomical Union Circular (1930): 2. Bibcode:1965IAUC.1930....2W.
  12. ↑ "SN 1965L". Transient Name Server. IAU . Retrieved 1 December 2024.
  13. ↑ Nakano, S.; Kushida, R.; Koshida, Y.; Garnavich, P.; Challis, P.; Kirshner, R.; Hergenrother, C.; Brown, W.; Marzke, R.; Odewahn, S. (1996). "Supernova 1996bu in NGC 3631". International Astronomical Union Circular (6505): 1. Bibcode:1996IAUC.6505....1N.
  14. ↑ "SN 1996bu". Transient Name Server. IAU . Retrieved 1 December 2024.
  15. ↑ "SN 2016bau". Transient Name Server. IAU . Retrieved 1 December 2024.
  16. ↑ Granata, V.; Benetti, S.; Cappellaro, E.; Elias-Rosa, N.; Pastorello, A.; Tomasella, L.; Nascimbeni, V.; Ochner, P.; Tartaglia, L.; Terreran, G.; Turatto, M. (March 15, 2016). "Asiago spectroscopic and photometric observations of AT2016bau". The Astronomer's Telegram. 8818: 1. Bibcode:2016ATel.8818....1G.
  17. ↑ Kamble, Atish; Margutti, Raffaella; Alexander, Kate; Berger, Edo; Cantiello, Matteo; Challis, Pete; Chomiuk, Laura; Guidorzi, Christiano; Kirshner, Robert; Milisavljevic, Danny; De Mink, Selma; Parrent, Jerod; Soderberg, Alicia; Zapartas, Emmanouil; Zauderer, Ashley (April 5, 2016). "VLA observations of SN 2016bau of Type Ib in NGC 3631". The Astronomer's Telegram. 8911: 1. Bibcode:2016ATel.8911....1K.
  18. ↑ 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.
  19. 1 2 "The Ursa Major Groups". www.atlasoftheuniverse.com.
  20. ↑ Tully, R. Brent (1988). Nearby galaxies catalog (1. publ ed.). Cambridge: Cambridge University Press. ISBN   978-0-521-35299-4.
  21. ↑ Karachentsev, I. D.; Nasonova, O. G.; Courtois, H. M. (March 2013). "Anatomy of Ursa Majoris". Monthly Notices of the Royal Astronomical Society. 429 (3): 2264–2273. arXiv: 1211.5975 . Bibcode:2013MNRAS.429.2264K. doi: 10.1093/mnras/sts494 . ISSN   0035-8711.
  22. ↑ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
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