Jump to content

NGC 3621

Coordinates: Sky map 11h 18m 16.5109s, −32° 48′ 49.732″
From Wikipedia, the free encyclopedia
NGC 3621
NGC 3621 taken by the Wide Field Imager (WFI) at ESO's La Silla Observatory
Observation data (J2000 epoch)
ConstellationHydra
Right ascension11h 18m 16.5109s[1]
Declination–32° 48′ 49.732″[1]
Redshift0.002403[1]
Heliocentric radial velocity720 ± 0 km/s[1]
Distance21.7 million light years (6.64 Mpc)[2]
Apparent magnitude (V)9.56[3]
Characteristics
TypeSA(s)d[4]
Mass2 × 1010[4] M☉
Size~216,900 ly (66.49 kpc) (estimated)[1]
Apparent size (V)10.96′ × 4.79′[3]
Other designations
ESO 377- G 037, IRAS 11158-3232, UGCA 232, MCG -05-27-008, PGC 34554[3][1]

NGC 3621 is a field spiral galaxy about 22 Mly (6.7 Mpc) away[2][5] in the equatorial constellation of Hydra. It was discovered by German-British astronomer William Herschel on 17 February 1790.[6]

NGC 3621 is comparatively bright and can be well seen in moderate-sized telescopes. The galaxy is around 216,900 ly (66,500 pc)[1] across and is inclined at an angle of 66° from being viewed face on.[7] It shines with a luminosity equal to 13 billion times that of the Sun.[8] The morphological classification is SA(s)d,[4] which indicates this is an ordinary spiral with loosely wound arms.[9] There is no evidence for a bulge.[10] Although it appears to be isolated,[9] NGC 3621 belongs to the Leo spur.[8]

This galaxy has an active nucleus that matches a Seyfert 2 optical spectrum, suggesting that a low mass supermassive black hole is present at the core. Based upon the motion of stars in the nucleus, this object may have a mass of up to three million times the mass of the Sun.[10]

One supernova has been observed in NGC 3621: SN 2024ggi (type II, mag. 18.915)[11] was discovered by ATLAS on 11 April 2024, and by 16 April it had brightened to magnitude 12. It is the closest supernova to Earth since SN 2023ixf, which was discovered on 19 May 2023. A search of archival Hubble Space Telescope and Spitzer Space Telescope images showed the suspected progenitor star, identified as a red supergiant.[12]

[edit]

See also

[edit]

References

[edit]
  1. ^ a b c d e f g "Results for object NGC 3621". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 5 December 2024.
  2. ^ a b Tully, R. Brent; et al. (March 2008), "Our Peculiar Motion Away from the Local Void", The Astrophysical Journal, 676 (1): 184–205, arXiv:0705.4139, Bibcode:2008ApJ...676..184T, doi:10.1086/527428, S2CID 14738309.
  3. ^ a b c "NGC 3621". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-24.
  4. ^ a b c Bresolin, Fabio; Kennicutt, Robert C.; Ryan-Weber, Emma (May 2012), "Gas Metallicities in the Extended Disks of NGC 1512 and NGC 3621. Chemical Signatures of Metal Mixing or Enriched Gas Accretion?", The Astronomical Journal, 750 (2): 122, arXiv:1203.0956, Bibcode:2012ApJ...750..122B, doi:10.1088/0004-637X/750/2/122, S2CID 118616035.
  5. ^ Materne, J. (April 1979). "The structure of nearby groups of galaxies - Quantitative membership probabilities". Astronomy and Astrophysics. 74 (2): 235–243. Bibcode:1979A&A....74..235M.
  6. ^ Seligman, Courtney. "New General Catalogue Objects: NGC 3621". Celestial Atlas. Retrieved 5 December 2024.
  7. ^ Lang, Philipp (July 2020), "PHANGS CO Kinematics: Disk Orientations and Rotation Curves at 150 pc Resolution", The Astrophysical Journal, 897 (2): 122, arXiv:2005.11709, Bibcode:2020ApJ...897..122L, doi:10.3847/1538-4357/ab9953.
  8. ^ a b O'Meara, Stephen James (2013), Deep-Sky Companions: Southern Gems, Cambridge University Press, p. 203, Bibcode:2013dcsg.book.....O, ISBN 978-1107015012.
  9. ^ a b Buta, Ronald J.; Corwin, Harold G.; Odewahn, Stephen C. (2007), Atlas of Galaxies, Cambridge University Press, pp. 13–17, ISBN 978-0521820486.
  10. ^ a b Barth, Aaron J.; Strigari, Louis E.; Bentz, Misty C.; Greene, Jenny E.; Ho, Luis C. (January 2009), "Dynamical Constraints on the Masses of the Nuclear Star Cluster and Black Hole in the Late-Type Spiral Galaxy NGC 3621", The Astronomical Journal, 690 (1): 1031–1044, arXiv:0809.1066, Bibcode:2009ApJ...690.1031B, doi:10.1088/0004-637X/690/1/1031, S2CID 12574940.
  11. ^ "SN 2024ggi". Transient Name Server. IAU. Retrieved 4 December 2024.
  12. ^ Xiang, Danfeng; Mo, Jun; Wang, Xiaofeng; Wang, Lingzhi; Zhang, Jujia; Lin, Han; Chen, Liyang; Song, Cuiying; Liu, Liang-Duan; Wang, Zhenyu; Li, Gaici (2024). "The Red Supergiant Progenitor of Type II Supernova 2024ggi". The Astrophysical Journal. 969 (1): L15. arXiv:2405.07699. Bibcode:2024ApJ...969L..15X. doi:10.3847/2041-8213/ad54b3.
  13. ^ "A special spiral galaxy for over 200 000 Facebook fans". Hubble Space Telescope – Picture of the Week. Retrieved 23 January 2020.
  14. ^ "A galaxy full of surprises — NGC 3621 is bulgeless but has three central black holes". European Southern Observatory – Picture of the Week. Retrieved 23 January 2020.
[edit]
Wikimedia Commons has media related to NGC 3621.
Stub icon

This spiral galaxy article is a stub. You can help Wikipedia by expanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=NGC_3621&oldid=1261353822"