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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 2(483), p. 2014-2030, 2018

DOI: 10.1093/mnras/sty2971

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Modelling the abundance structure of isocyanic acid (HNCO) towards the low-mass solar type protostar IRAS 16293–2422

Journal article published in 2018 by Antonio Hernández-Gómez ORCID, Emna Sahnoun ORCID, Emmanuel Caux ORCID, Laurent Wiesenfeld ORCID, Laurent Loinard ORCID, Sandrine Bottinelli ORCID, Kamel Hammami ORCID, Karl M. Menten ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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