arXiv · astro-ph/0307001
PSR B1849+00 probes the tiny-scale molecular gas?
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.
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S. Stanimirovic, J. M. Weisberg, J. M. Dickey, A. de la Fuente, K. Devine, A. Hedden, S. B. Anderson. 2003-06-30. PSR B1849+00 probes the tiny-scale molecular gas?. https://doi.org/10.1023/b%3Aastr.0000045014.63134.97
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