The pressure-confined wind of the massive and compact super star cluster M82-A1

The observed parameters of the young super star cluster M82-A1 and its associated compact H 🇮🇮 region are here shown to indicate a low heating efficiency or immediate loss, through radiative cooling, of a large fraction of the energy injected by stellar winds and supernovae during the early evolutio...

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Bibliographic Details
Main Authors: SERGIY SILICH, GUILLERMO TENORIO TAGLE
Format: info:eu-repo/semantics/article
Language:eng
Published: The astrophysical journal 2007
Subjects:
Online Access:http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1003

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