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The Physics of Disk Winds
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The Physics of Disk Winds

Abstract

The last decade of research on star formation has established two important facts, namely that most if not all young stellar objects (henceforth YSO’s) are associated with both outflows and disks. The obvious question is whether or not these two phenomena are physically related. The outflow data clearly show that radiation cannot be the driving agent for the outflows, so that hydromagnetic drives that employ rotation and strong magnetic fields …

Authors

Pudritz RE; Pelletier G; Gomez de Castro AI

Pagination

pp. 539-564

Publisher

Springer Nature

Publication Date

1991

DOI

10.1007/978-94-011-3642-6_16

Conference proceedings

Nato Science Series C:

ISSN

1389-2185