Superbubble Activity in Star-Forming Galaxies

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dc.creatorOey, M. S.
dc.date2002-12-03
dc.date.accessioned2026-07-07T10:31:33Z
dc.date.available2026-07-07T10:31:33Z
dc.descriptionMechanical feedback from massive stars, primarily from supernovae, can dominate ISM structuring and phase balance, thereby profoundly affecting galactic evolutionary processes. Our understanding of mechanical feedback is based on the adiabatic, wind-driven bubble model, applied on size scales ranging over three decades. Tests of the model, and our consequent understanding of feedback, are reviewed. While the model is broadly successful, critical unknowns still prevent a comprehensive understanding of the consequences of feedback.
dc.description10 pp., uses kluwer.cls. Invited Review to appear in "From Observations to Self-Consistent Modelling of the ISM in Galaxies, eds. M. A. de Avillez & D. Breitschwerdt, JENAM 2002 WS-ISM, (Kluwer) Ap&SS, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0212051
dc.identifierhttp://arxiv.org/abs/astro-ph/0212051
dc.identifierAstrophys.SpaceSci.289:269-277,2004
dc.identifierdoi:10.1023/B:ASTR.0000014954.00889.ad
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178450
dc.subjectAstrophysics
dc.titleSuperbubble Activity in Star-Forming Galaxies
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