F06296$+$5743 : A Very Massive Starburster ?
Astrophysics
2007-05-23 v1
Abstract
We have observed an object having strong Balmer absorption lines and blue continuum. The inference about the nuclear stellar population drawn from the line ratios is basically coincident with that drawn from the continuum color, both indicating the dominant fraction of early A type population in the nucleus. This might be expected only if there has been a very massive starburst, burst strength of 10\% at least.
Keywords
Cite
@article{arxiv.astro-ph/9604058,
title = {F06296$+$5743 : A Very Massive Starburster ?},
author = {J. H. Huang and Q. S. Gu and H. J. Su and Z. H. Shang},
journal= {arXiv preprint arXiv:astro-ph/9604058},
year = {2007}
}
Comments
4 pages, l-aa.sty, 1 figure available on request at jhh@nju.edu.cn, accepted for publication in A\&A