Chemical evolution of spiral galaxies: models with star formation proportional to molecular hydrogen

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dc.contributor.author Tosi, M.
dc.contributor.author Díaz, Angeles I.
dc.date.accessioned 2014-02-18T09:50:20Z
dc.date.available 2013-07-10
dc.date.issued 1990
dc.identifier.citation Monthly Notices of the Royal Astronomical Society 246 (1990): 616-623
dc.identifier.issn 1365-2966
dc.identifier.uri http://hdl.handle.net/10486/13347
dc.description This is an electronic version of an article published in Monthly Notices of the Royal Astronomical Society. Tosi, M., Díaz, A.I. Chemical evolution of spiral galaxies: models with star formation proportional to molecular hydrogen. Monthly Notices of the Royal Astronomical Society 246 (1990): 616-623
dc.format.mimetype Application/pdf
dc.language.iso eng
dc.publisher Oxford University Press
dc.rights © Royal Astronomical Society
dc.subject Galaxies: spiral
dc.title Chemical evolution of spiral galaxies: models with star formation proportional to molecular hydrogen
dc.type article
dc.subject.eciencia Física
dc.type.review Peer reviewed
dc.rights.accessRights openAccess en
dc.authorUAM Díaz Beltrán, Ángeles Isabel (259696)


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