NGC 7603 explained

NGC 7603
Epoch:J2000.0
Constellation Name:Pisces
Size V:1.5 × 1.0 moa
Appmag V:14.04
Type:SA(rs)b: pec Sy1.5
Dist Ly:412.9+/-[1]
Names:NGC 7603, UGC 12493, MCG 0-59-21, MK 530, PGC 71035, IRAS23163-0001, UM 156, ARP 92, ZWG 380.26[2]
References:NGC+7603[3]

NGC 7603 is a spiral Seyfert galaxy in the constellation Pisces. It is listed (as Arp 92) in the Atlas of Peculiar Galaxies.[4] It is interacting with the smaller elliptical galaxy PGC 71041 nearby.

This galaxy pair has long been a cornerstone for those who are critical of the view that the universe is expanding, and advocates for non-standard cosmology such as Halton Arp, Fred Hoyle, and others.[5] [6] This is due to the position of two quasars, one at each edge of the filament connecting the two galaxies, with much more redshift than either galaxy.

External links

Notes and References

  1. NGC 7603 . 6 July 2017.
  2. Web site: Revised NGC Data for NGC 4889. spider.seds.org. 2015-10-13.
  3. Web site: NASA/IPAC Extragalactic Database . Results for object NGC 7603 . 2017-07-06 .
  4. Web site: ARP Atlas of Peculiar Galaxies 89-92. ARP ATLAS OF PECULIAR GALAXIES. 7 July 2017.
  5. Web site: NGC 7603. Quasars.org. 3 December 2018. https://web.archive.org/web/20181012015801/http://quasars.org/ngc7603.htm. 12 October 2018. dead.
  6. Web site: Universe: The Cosmology Quest 1 of 2. Youtube. 3 December 2018.