NGC 4697 explained

NGC 4697
Epoch:J2000
Constellation Name:Virgo
Type:E6[1]
Dist Ly:~ 38 Mly / ~ 50 Mly[2]
Z:1241 ± 1 km/s
Size V:4.4 × 2.8
Appmag V:10.97
Names:Caldwell 52, UGCA 300, MCG -01-33-010, PGC 043276

NGC 4697 (also known as Caldwell 52) is an elliptical galaxy some 40 to 50 million light-years away in the constellation Virgo. It is a member of the NGC 4697 Group, a group of galaxies also containing NGC 4731 and several generally much smaller galaxies.[3] This group is about 55 million light-years away; it is one of the many Virgo II Groups, which form a southern extension of the Virgo Supercluster of galaxies.

The distance to NGC 4697 is not known with high precision: measurements vary from 28 to 76 million light-years. According to the NASA Extra-galactic Database, the average is about 38 million light-years; according to SIMBAD, about 50 million light-years.

The supermassive black hole at the core of NGC 4697 has a mass of as measured from Atacama Large Millimeter Array observations of the rotation of the central gas disk.[4]

One supernova has been observed in NGC 4697: SN 2018imd (type Ia, mag. 15.5).[5]

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . NED results for object NGC 4697 . 2010-11-28 .
  2. NGC 4697 . 2010-11-28 .
  3. Web site: The Virgo II Groups . Atlas of the Universe . 2010-11-28 .
  4. Davis . T. A. . Bureau . M. . Onishi . K. . Cappellari . M. . Iguchi . S. . Sarzi . M. . WISDOM Project - II. Molecular gas measurement of the supermassive black hole mass in NGC 4697 . Monthly Notices of the Royal Astronomical Society . 2017 . 468 . 4 . 4675 . 10.1093/mnras/stw3217 . free . 2017MNRAS.468.4675D. 1703.05248 .
  5. https://www.wis-tns.org/object/2018imd Transient Name Server entry for SN 2018imd.