Theory and Extragalactic Masers
Abstract
Theoretical research on extragalactic masers (and hence this review) is almost entirely directed toward 22 GHz water masers in circumnuclear disks with the focus being the near ideal masing disk at the nucleus of the galaxy NGC4258. The discussion here is organized around (1) the excitation and conditions for the masers, (2) the spatial and spectral appearance of the maser emission, and (3) the mass accretion rate and structure of the disk. In addition, a summary is given of the basic physics (spectral linebeadths and maser polarization) that underlies certain interpretations of these and other astrophysical masers.
Keywords
Cite
@article{arxiv.astro-ph/0107572,
title = {Theory and Extragalactic Masers},
author = {William D. Watson},
journal= {arXiv preprint arXiv:astro-ph/0107572},
year = {2007}
}
Comments
to appear in the proceedings of IAU Symposium #206: Cosmic Masers (Mangaratiba, Brazil; March 2001); 16 pages; 5 figures; uses newpasp.sty