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The abundances of nitrogen-containing molecules during pre-protostellar collapse

2006/07/06 by D. R. Flower, G. Pineau des Forêts, G. Pineau des Forets +1 · 1 citation
Chemistry · Physics and Astronomy · #Advanced Chemical Physics Studies #Astrophysics and Star Formation Studies #Molecular Spectroscopy and Structure #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065375

22 Pages, 7 Figures, Accepted by Astronomy and Astrophysics

arxiv created 2006/07/06 · openalex publication_date 2006/08/04 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/28

Abstract

Aims.We have studied the chemistry of nitrogen-bearing species during the initial stages of protostellar collapse, with a view to explaining the observed longevity of N2H+ and NH3 and the high levels of deuteration of these species.

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