HCG 87 explained

HCG 87 is a compact group of galaxies listed in the Hickson Compact Group Catalogue. This group is about 400 million light-years away [1] in the constellation Capricornus. The group distinguishes itself as one of the most compact groups of galaxies, hosting two active galactic nuclei and a starburst among its three members, all of which show signs of interaction.[2] This interaction, which astronomers have called visually, and scientifically, intriguing[3] is being examined to understand the influence of active nuclei on star formation histories.

Members

Members of the HCG 87
NameType[4] R.A. (J2000)Dec. (J2000)Redshift (km/s)Apparent Magnitude
HCG 87aS0 pec8443 ± 1415.3
HCG 87bSA(r)0 pec8740 ± 2015.4
HCG 87cSb8914 ± 716.1
HCG 87dSd10200 ± 16017.8

External links

Notes and References

  1. Web site: This redshift corresponds to a distance of 120Mpc or 400 million light years (using H0 = 75km/s/Mpc and q0 = 0.1). At the distance of the group, this corresponds to a group diameter of 52kpc, i.e., the group is approximately 170,000 light years across . dead . 19 February 2020 . https://web.archive.org/web/20200219030953/http://heritage.stsci.edu/1999/31/hicktable.ps . PS File download need Photoshop or GIMP .
  2. Noll, Keith. 07/1999. "Hubble Heritage observations of Hickson Compact Galaxy Group 87".
  3. English, J. et al. 05/2000. "A Minuet of Galaxies: Hickson Compact Group 87 as Viewed by the Hubble Space Telescope". American Astronomical Society, 195th AAS Meeting, #136.04; Bulletin of the American Astronomical Society, Vol. 32, p.884.
  4. Web site: NASA/IPAC Extragalactic Database . Results for various galaxies . 2006-10-19.