Neutral Hydrogen in Arp 158
Abstract
We present 21 cm observations of Arp 158. We have performed a study of the neutral hydrogen (H I) to help us understand the overall formation and evolution of this system. This is a disturbed system with distinct optical knots connected by a linear structure embedded in luminous material. There is also a diffuse spray to the southeast. The H I seems to be made up of three distinct, kinematically separate systems. Arp 158 bears a certain optical resemblance to NGC 520 (Arp 157), which has been identified as a mid-stage merger. From our 21 cm observations of Arp 158, we also see a comparable H I content with NGC 520. These similarities suggest that Arp 158 is also an intermediate-stage merger.
- Publication:
-
The Astronomical Journal
- Pub Date:
- September 2004
- DOI:
- 10.1086/422731
- arXiv:
- arXiv:astro-ph/0405405
- Bibcode:
- 2004AJ....128..985I
- Keywords:
-
- galaxies: individual (Arp 158);
- Galaxies: Interactions;
- ISM: Abundances;
- Astrophysics
- E-Print:
- 11 pages, 16 figures. Accepted for publication in AJ