PSR B1849+00 探测微尺度分子气体？
天体物理学
2008-11-26 v1
摘要
本文报告并讨论了PSR B1849+00 与 SNR G33.6+0.1 沿相同视线的 OH 吸收光谱之间的巨大差异。此发现至关重要，因为它清楚地表明分子气体的吸收统计性质取决于背景源的尺寸。
引用
@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}
}
备注
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