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Composition Gradients in Spiral Galaxies

Published online by Cambridge University Press:  30 March 2016

Manuel Peimbert
Manuel Peimbert*
Affiliation:
Instituto de Astronomía, UNAM Apartado Postal 70-264, México 01510, D. F.

Extract

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Some topics on composition gradients are discussed. One of the most important processes responsible for the abundance gradients is the variation of the low-mass end of the IMF with O/H.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 10: Highlights of Astronomy. As presented at the XXIInd General Assembly of the IAU, 1994 , 1995 , pp. 486 - 489
Copyright
Copyright © Kluwer 1995

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