Interstellar chemistry of nitrogen hydrides in dark clouds
about
Concluding remarks: astrochemistry of dust, ice and gas.H2D(+) observations give an age of at least one million years for a cloud core forming Sun-like stars.Reaction between HN and SN: a possible channel for the interstellar formation of N2 and SH in the cold interstellar clouds.Rotational excitation of the interstellar NH2 radical by H2.
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Interstellar chemistry of nitrogen hydrides in dark clouds
description
article publié dans la revue scientifique Astronomy and Astrophysics
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im Februar 2014 veröffentlichter wissenschaftlicher Artikel
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scientific article published in Astronomy and Astrophysics
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wetenschappelijk artikel
@nl
наукова стаття, опублікована в лютому 2014
@uk
name
Interstellar chemistry of nitrogen hydrides in dark clouds
@en
Interstellar chemistry of nitrogen hydrides in dark clouds
@nl
type
label
Interstellar chemistry of nitrogen hydrides in dark clouds
@en
Interstellar chemistry of nitrogen hydrides in dark clouds
@nl
prefLabel
Interstellar chemistry of nitrogen hydrides in dark clouds
@en
Interstellar chemistry of nitrogen hydrides in dark clouds
@nl
P2093
P2860
P356
P1476
Interstellar chemistry of nitrogen hydrides in dark clouds
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G. Pineau des Forêts
P. Hily-Blant
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P356
10.1051/0004-6361/201322386
P407
P577
2014-02-01T00:00:00Z
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P819
2014A&A...562A..83L