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

Simple item page
dc.creatorStanimirovic, S.
dc.creatorWeisberg, J. M.
dc.creatorDickey, J. M.
dc.creatorde la Fuente, A.
dc.creatorDevine, K.
dc.creatorHedden, A.
dc.creatorAnderson, S. B.
dc.date2003-06-30
dc.date.accessioned2026-07-07T10:27:00Z
dc.date.available2026-07-07T10:27:00Z
dc.descriptionIn 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.
dc.descriptionTo 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0307001
dc.identifierhttp://arxiv.org/abs/astro-ph/0307001
dc.identifierAstrophys.SpaceSci.292:167-172,2004
dc.identifierdoi:10.1023/B:ASTR.0000045014.63134.97
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177030
dc.subjectAstrophysics
dc.titlePSR B1849+00 probes the tiny-scale molecular gas?
dc.typetext

Files

Collections

arXiv