Misplaced Pages

NGC 4790

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Galaxy in the constellation Virgo
NGC 4790
NGC 4790 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12 54 51.956
Declination−10° 14′ 52.2″
Redshift0.004483
Heliocentric radial velocity1344 ± 5 km/s
Distance80.8 ± 5.8 Mly (24.76 ± 1.77 Mpc)
Group or clusterNGC 4699 Group
Apparent magnitude (V)12.4
Characteristics
TypeSB(rs)c?
Size~45,500 ly (13.95 kpc) (estimated)
Apparent size (V)1.55′ × 1.0′
Other designations
IRAS 12522-0958, MCG -02-33-056, PGC 43972

NGC 4790 is a barred spiral galaxy located in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 1679 ± 24 km/s, which corresponds to a Hubble distance of 80.8 ± 5.8 Mly (24.76 ± 1.77 Mpc). In addition, six non-redshift measurements give a distance of 74.75 ± 4.07 Mly (22.917 ± 1.249 Mpc). It was discovered on 25 March 1786 by German-British astronomer William Herschel.

NGC 4790 is a member of the NGC 4699 Group (also known as LGG 307) of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.

One supernova has been observed in NGC 4790. SN 2012au (type Ib, mag. 13.8) was discovered by the Catalina Sky Survey on 14 March 2012. This supernova later produced evidence of a pulsar wind nebula which appears to be expanding outward at approximately 2300 km/s.

See also

References

  1. ^ "Results for object NGC 4790". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 25 November 2024.
  2. "Distance Results for NGC 4790". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 25 November 2024.
  3. Seligman, Courtney. "New General Catalogue Objects: NGC 4790". Celestial Atlas. Retrieved 25 November 2024.
  4. "The Virgo III Groups". Atlas of the Universe. Retrieved 2010-11-27.
  5. 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.
  6. "SN 2012au". Transient Name Server. IAU. Retrieved 25 November 2024.
  7. SN 2012au at rochesterastronomy.com
  8. Milisavljevic, Dan; Patnaude, Daniel J.; Chevalier, Roger A.; Raymond, John C.; Fesen, Robert A.; Margutti, Raffaella; Conner, Brody; Banovetz, John (2018). "Evidence for a Pulsar Wind Nebula in the Type Ib Peculiar Supernova SN 2012au". The Astrophysical Journal Letters. 864 (2): L36. arXiv:1809.01141. Bibcode:2018ApJ...864L..36M. doi:10.3847/2041-8213/aadd4e.

External links

Galaxies
Morphology
Structure
Active nuclei
Energetic galaxies
Low activity
Interaction
Lists
See also
New General Catalogue 4500 to 4999
Constellation of Virgo
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Galaxies
Messier
NGC
Other
Galaxy clusters
Astronomical events
Category
Portals:
Stub icon

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

Categories: