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- Q1110494 subject Q1031119.
- Q1110494 subject Q7033665.
- Q1110494 subject Q7152550.
- Q1110494 subject Q7215991.
- Q1110494 abstract "NGC 4293 is the New General Catalogue identifier for a lenticular galaxy in the northern constellation of Coma Berenices. It was discovered by English astronomer William Herschel on March 14, 1784, who described it as "large, extended, resolvable, 6 or 7′ long". This galaxy is positioned to the north-northwest of the star 11 Comae Berenices and is a member of the Virgo Cluster of galaxies. It is assumed to lie at the same distance as the Virgo Cluster itself: around 54 million light years away. The galaxy spans an apparent area of 5.3 × 3.1 arc minutes.The morphological classification of NGC 4293 is (R)SB(s)0/a, with the SB0/a indicating this has just distinguishable tightly wound spiral arms with a bar structure at the nucleus. An '(s)' notation means that this galaxy does not have a ring-like structure around the nucleus. Star formation within NGC 4293 is only taking place within a confined region at the center of the galaxy. The outer stellar disk of the galaxy appears disturbed, suggesting some form of gravitational interaction.This is a common type of active galaxy known as a LINER, which means that the optical spectrum is dominated by emission lines from gases in low energy ionization states. The activity may be the result of a supermassive black hole (SMBH) in the nucleus that is undergoing a low rate of matter accretion. The estimated mass of such an SMBH is 7007590000000000000♠5.9×107 M⊙. Radio emission from thermal activity has been detected from the proximity of this object.".
- Q1110494 thumbnail Ngc4293-hst-606.png?width=300.
- Q1110494 wikiPageWikiLink Q1031119.
- Q1110494 wikiPageWikiLink Q115462.
- Q1110494 wikiPageWikiLink Q14277.
- Q1110494 wikiPageWikiLink Q14534.
- Q1110494 wikiPageWikiLink Q1648748.
- Q1110494 wikiPageWikiLink Q180892.
- Q1110494 wikiPageWikiLink Q192078.
- Q1110494 wikiPageWikiLink Q212111.
- Q1110494 wikiPageWikiLink Q22066400.
- Q1110494 wikiPageWikiLink Q2490.
- Q1110494 wikiPageWikiLink Q2513.
- Q1110494 wikiPageWikiLink Q2557101.
- Q1110494 wikiPageWikiLink Q2703.
- Q1110494 wikiPageWikiLink Q271818.
- Q1110494 wikiPageWikiLink Q36496.
- Q1110494 wikiPageWikiLink Q40392.
- Q1110494 wikiPageWikiLink Q4547758.
- Q1110494 wikiPageWikiLink Q46587.
- Q1110494 wikiPageWikiLink Q531.
- Q1110494 wikiPageWikiLink Q615925.
- Q1110494 wikiPageWikiLink Q6709611.
- Q1110494 wikiPageWikiLink Q7033665.
- Q1110494 wikiPageWikiLink Q7152550.
- Q1110494 wikiPageWikiLink Q7215991.
- Q1110494 wikiPageWikiLink Q724913.
- Q1110494 wikiPageWikiLink Q8928.
- Q1110494 wikiPageWikiLink Q9285.
- Q1110494 name "NGC 4293".
- Q1110494 names "2".
- Q1110494 type Place.
- Q1110494 type CelestialBody.
- Q1110494 type Galaxy.
- Q1110494 type Location.
- Q1110494 type Place.
- Q1110494 type Thing.
- Q1110494 type Q318.
- Q1110494 comment "NGC 4293 is the New General Catalogue identifier for a lenticular galaxy in the northern constellation of Coma Berenices. It was discovered by English astronomer William Herschel on March 14, 1784, who described it as "large, extended, resolvable, 6 or 7′ long". This galaxy is positioned to the north-northwest of the star 11 Comae Berenices and is a member of the Virgo Cluster of galaxies. It is assumed to lie at the same distance as the Virgo Cluster itself: around 54 million light years away.".
- Q1110494 label "NGC 4293".
- Q1110494 depiction Ngc4293-hst-606.png.
- Q1110494 name "2MASXJ12211289+1822566,IRAS12186+1839,LEDA39907,UGC7405,UZCJ122112.6+182256,Z99-23.".
- Q1110494 name "NGC 4293".