PSR B1849+00 probes the tiny-scale molecular gas?

Astronomy and Astrophysics – Astrophysics

Scientific paper

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To be published in the proceedings of "Magnetic fields and star formation: theory versus observations", held in Madrid, April

Scientific paper

10.1023/B:ASTR.0000045014.63134.

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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