About the central regions of the IrrII galaxies - the members of tight groups and chains.
Abstract
The abundance of the objects with splitted nuclei among the candidates - the members of tight systems can be explained by the existence of bright H II regions in their central parts and also by the existence of dust lanes in their nuclear regions.
- Publication:
-
Publications of the Astronomical Institute of the Czechoslovak Academy of Sciences
- Pub Date:
- 1987
- Bibcode:
- 1987PAICz..69..343I
- Keywords:
-
- Galactic Structure;
- H Ii Regions;
- Irregular Galaxies;
- Astronomical Catalogs;
- Cosmic Dust;
- Galactic Nuclei;
- Astrophysics;
- Active Galaxies:Irregular Galaxies;
- Galactic Centers:H II Regions;
- Galactic Centers:Irregular Galaxies;
- Galaxy Groups:Irregular Galaxies;
- H II Regions:Galactic Centers;
- Irregular Galaxies:Active Galaxies;
- Irregular Galaxies:Galactic Centers;
- Irregular Galaxies:Galaxy Groups