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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 2(456), p. 1269-1293, 2015

DOI: 10.1093/mnras/stv2651

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Modelling supernova line profile asymmetries to determine ejecta dust masses: SN 1987A from days 714 to 3604

Journal article published in 2015 by Antonia Bevan ORCID, M. J. Barlow 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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