Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/10261/2613
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dc.creatorDaniel, Fabien-
dc.creatorCernicharo, José-
dc.creatorRoueff, E.-
dc.creatorGerin, M.-
dc.creatorDubernet, M. L.-
dc.date2007-12-27T08:52:09Z-
dc.date2007-12-27T08:52:09Z-
dc.date2007-06-06-
dc.date.accessioned2017-01-31T00:59:32Z-
dc.date.available2017-01-31T00:59:32Z-
dc.identifierarXiv:0706.0802v1-
dc.identifierhttp://hdl.handle.net/10261/2613-
dc.identifier.urihttp://dspace.mediu.edu.my:8181/xmlui/handle/10261/2613-
dc.descriptionAccepted for publication in The Astrophysical Journal (ApJ).-
dc.descriptionWe present observations of the J=1-0, 2-1, and 3-2 rotational transitions of N2H+ and N2D+ towards a sample of prototypical dark clouds. The data have been interpreted using non-local radiative transfer models.-
dc.descriptionThe authors acknowledge funding support under grants PNAYA2000-1784, ESP2001-4516, PNAYA2002-10113-E, ESP2002-01627, PNAYA2003-02785, PNAYA2004-0579 and the Madrid DGU PRICIT Program S-0505/ESP-0237 (ASTROCAM).-
dc.descriptionPeer reviewed-
dc.format1131814 bytes-
dc.formatapplication/pdf-
dc.languageeng-
dc.relationPreprint-
dc.rightsopenAccess-
dc.subjectLine: formation: profiles-
dc.subjectMolecular processes-
dc.subjectRadiative transfer-
dc.subjectISM: clouds: molecules: abundances-
dc.subjectISM: individual (TMC1, L183)-
dc.titleN2H+ and N2D+ in interstellar molecular clouds. II- Observations-
dc.typePre-print-
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