The Evolving XUV Absorber in NGC3516
Astrophysics
2007-05-23 v1
Abstract
For NGC3516 we find that the X-ray warm absorption and the broad UV associated absorption features can be produced by the same absorbing material. We argue that the evolution of the XUV absorber from pre-1992 to 1995 is consistent with expectation for an expanding, outflowing material.
Cite
@article{arxiv.astro-ph/9608007,
title = {The Evolving XUV Absorber in NGC3516},
author = {Smita Mathur and Belinda Wilkes and Thomas Aldcroft},
journal= {arXiv preprint arXiv:astro-ph/9608007},
year = {2007}
}
Comments
2 pages, 1 figure. Uses aspconf.sty, included. To be published in the Proceedings of IAU Colloquium 159 on "Emission Lines in Active Galaxies: New Methods and Techniques"