pith. sign in

arxiv: astro-ph/0211139 · v1 · submitted 2002-11-07 · 🌌 astro-ph

The nature of the ultraluminous X-ray sources inside galaxies and their relation to local QSOs

classification 🌌 astro-ph
keywords galaxieslocalqsossourcesthoseultraluminousx-rayactive
0
0 comments X
read the original abstract

It is suggested that many of the ultraluminous compact x-ray sources now being found in the main bodies of galaxies, particularly those that are active, like M82, NGC 3628 and others, are "local" QSOs, or BL Lac objects, with high intrinsic redshifts in the process of being ejected from those galaxies. Evidence in support of this hypothesis is summarized.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.