Universidad Autónoma de Madrid

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

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

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Título: Chemical evolution of spiral galaxies: models with star formation proportional to molecular hydrogen
Autor (es): Tosi, M.; Díaz, Angeles I.
Editor: Oxford University Press
Fecha de edición: 1990
Cita: Monthly Notices of the Royal Astronomical Society 246 (1990): 616-623
ISSN: 1365-2966
Materias: Galaxies: spiral; Física
URI: http://hdl.handle.net/10486/13347
Nota: 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
Derechos: © Royal Astronomical Society

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G o o g l e ™ Scholar: Tosi, M. - Díaz, Angeles I.

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