MS 0129.2-2237: Interacting Galaxies at Z = 0.11
Abstract
The x-ray source MS 0129.2 - 2237 is positionally coincident with an interacting system of galaxies. We present the results of our spectroscopic and photometric investigation of the system, which show that a Seyfert 1.5, a Seyfert 2 nucleus or H II region or a starburst galaxy, a normal galaxy plus possibly another galaxy where star-forming activity is taking place are strongly interacting. The redshift of the system is z = 0.11. The maximum projected diameter of the envelope common to the four spectroscopi- cally distinct objects is ~98 kpc (H_0_ = 50 km s^-1^ Mpc^-1^ and q_0_ = 0.5). The isolated environment in which the system lies suggests that we are looking at the final stage of the life of a compact group of galaxies where members are merging into an elliptical galaxy.
- Publication:
-
The Astronomical Journal
- Pub Date:
- November 1990
- DOI:
- Bibcode:
- 1990AJ....100.1461M
- Keywords:
-
- Elliptical Galaxies;
- Galactic Clusters;
- Galactic Evolution;
- Interacting Galaxies;
- Multispectral Band Scanners;
- Astronomical Photometry;
- Astronomical Spectroscopy;
- H Ii Regions;
- Seyfert Galaxies;
- Starburst Galaxies;
- X Ray Sources;
- Astrophysics;
- GALAXIES: INTERACTIONS;
- GALAXIES: INDIVIDUAL