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

(2) Carleton College; (3) University of Minnesota; (4) Caltech); A. de la Fuente; A. Hedden (2); J.M. Dickey (3); J.M. Weisberg (2); K. Devine; S.B. Anderson (4) ((1) UC Berkeley; S. Stanimirovic (1)

arxiv: astro-ph/0307001 · v1 · submitted 2003-06-30 · 🌌 astro-ph

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

S. Stanimirovic (1) , J.M. Weisberg (2) , J.M. Dickey (3) , A. de la Fuente , K. Devine , A. Hedden (2) , S.B. Anderson (4) ((1) UC Berkeley , (2) Carleton College

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(3) University of Minnesota (4) Caltech)

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classification 🌌 astro-ph

keywords b1849molecularabsorbingabsorptionalongbackgroundclearlydemonstrates

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

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