Svoboda | Graniru | BBC Russia | Golosameriki | Facebook

To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

NGC 2613
Observation data (J2000 epoch)
ConstellationPyxis
Right ascension08h 33m 22.841s[1]
Declination−22° 58′ 25.21″[1]
Redshift0.005591[2]
Heliocentric radial velocity1,675 km/s[3]
Distance78 Mly (24 Mpc)[3]
Apparent magnitude (V)11.6[2]
Characteristics
TypeSA(s)b[4]
Mass(7.50±0.87)×1011 M.[5] M
Apparent size (V)7′.59 × 1′.70[6]
Notable featuresEdge-on galaxy
Other designations
IRAS 08311-2248, MCG-04-21-003, UGCA 141, PGC 23997[7]

NGC 2613 is a spiral galaxy in the southern constellation of Pyxis, next to the western constellation border with Puppis. It was discovered by the German-born astronomer William Herschel on November 20, 1784.[8] With an apparent visual magnitude of 10.5, the galaxy is faintly visible using a telescope with a 100 mm (4 in) aperture. It appears spindle-shaped as it is almost edge-on to observers on Earth.[9]

The morphological classification of NGC 2613 is SA(s)b,[4] indicating a spiral galaxy with no bar or ring, and moderately tightly-wound spiral arms. It is inclined by an angle of approximately 79° to the line of sight from the Earth[5] and is oriented with the long axis along a position angle of 133°.[4] The radius of neutral hydrogen in the galaxy is about 35 kpc,[10] and the mass of the neutral hydrogen is (8.73±0.32)×109 M. The galaxy has a combined dynamic mass of (7.50±0.87)×1011 M.[5]

NGC 2613 has an active galactic nucleus that is deeply embedded in obscuring gas and dust.[5] Emission data collected by the Very Large Array shows a feature resembling a tidal tail along the southeast side of the galaxy, which was most likely produced by an interaction with the small companion galaxy, ESO 495-G017, now located to the northwest of NGC 2613.[10]

On 20 March 2023, a supernova was observed in NGC 2613: SN 2023dtc (Type Ib, mag. 18).[11]

References

  1. ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
  2. ^ a b "NASA/IPAC Extragalactic Database". Results for NGC 6946. Retrieved 22 September 2015.
  3. ^ a b Tully, R. Brent; et al. (August 2016). "Cosmicflows-3". The Astronomical Journal. 152 (2): 21. arXiv:1605.01765. Bibcode:2016AJ....152...50T. doi:10.3847/0004-6256/152/2/50. S2CID 250737862. 50.
  4. ^ a b c Chaves, Tara A.; Irwin, Judith A. (August 2001). "High-Latitude H I in NGC 2613: Structure and Dynamics". The Astrophysical Journal. 557 (2): 646–658. Bibcode:2001ApJ...557..646C. doi:10.1086/321686.
  5. ^ a b c d Li, Z.; et al. (September 2006). "An XMM-Newton observation of the massive edge-on Sb galaxy NGC 2613". Monthly Notices of the Royal Astronomical Society. 371 (1): 147–156. arXiv:astro-ph/0606543. Bibcode:2006MNRAS.371..147L. doi:10.1111/j.1365-2966.2006.10682.x. S2CID 1380874.
  6. ^ Paturel, G.; et al. (December 2003). "HYPERLEDA. I. Identification and designation of galaxies". Astronomy and Astrophysics. 412: 45–55. Bibcode:2003A&A...412...45P. doi:10.1051/0004-6361:20031411.
  7. ^ "NGC 2613". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-09-04.
  8. ^ Seligman, Courtney. "NGC Objects: NGC 2600 - 2649". Celestial Atlas. Retrieved 2020-09-05.
  9. ^ O'Meara, Stephen James (2007). Steve O'Meara's Herschel 400 Observing Guide. Cambridge, United Kingdom: Cambridge University Press. p. 82. ISBN 978-0-521-85893-9.
  10. ^ a b Irwin, Judith A.; Chaves, Tara (March 2003). "High-Latitude H I in NGC 2613: Buoyant Disk-Halo Outflow". The Astrophysical Journal. 585 (1): 268–280. arXiv:astro-ph/0212072. Bibcode:2003ApJ...585..268I. doi:10.1086/345891. S2CID 6400818.
  11. ^ Transient Name Server entry for SN 2023dtc. Retrieved 21 March 2023.

External links

This page was last edited on 3 December 2023, at 00:20
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.