ASPCS
 
Back to Volume
Paper: The HI Environment of Markarian 315
Volume: 240, Gas and Galaxy Evolution: A Conference in Honor of the 20th Anniversary of the VLA
Page: 408
Authors: Simkin, S. M.; MacKenty, J. W.
Abstract: Markarian 315 is a Seyfert galaxy with an ionized gas tail, ~70 kpc in length. We have mapped the extended HI gas associated with this galaxy and we find that the it is not associated with the ionized gas tail, but instead lies in a cloud located on the opposite (SSE) side of the galaxy at a projected distance of ~30 h-1 kpc.
Back to Volume