PSR B1849+00 probes the tiny-scale molecular gas?
Astrophysics
2008-11-26 v1
Abstract
In this paper we present and discuss the great difference in OH absorption spectra against PSR B1849+00 and SNR G33.6+0.1 along the same line-of-sight. This finding is important as it clearly demonstrates that statistics of absorbing molecular gas depends on the size of the background source.
Cite
@article{arxiv.astro-ph/0307001,
title = {PSR B1849+00 probes the tiny-scale molecular gas?},
author = {S. Stanimirovic and J. M. Weisberg and J. M. Dickey and A. de la Fuente and K. Devine and A. Hedden and S. B. Anderson},
journal= {arXiv preprint arXiv:astro-ph/0307001},
year = {2008}
}
Comments
To be published in the proceedings of "Magnetic fields and star formation: theory versus observations", held in Madrid, April 21-25 2003. Uses Kluwer style file