Cluster Formation and the ISM

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dc.creatorPudritz, Ralph E.
dc.creatorFiege, Jason D.
dc.date1999-05-12
dc.date.accessioned2026-07-25T13:34:04Z
dc.descriptionWe review the physics of star formation, and its links with the state of the ISM in galaxies. Current obervations indicate that the preferred mode of star formation is clustered. Given that OB associations provide the dominant energy input into the ISM, deep links exist between the ISM and star formation. We present a multi-scale discussion of star formation, and attempt to create an integrated vision of these processes.
dc.description13 pages, 1 figure. Conference proceeding (Naramata Workshop on the ISM, 1998)
dc.identifierhttps://arxiv.org/abs/astro-ph/9905149
dc.identifierhttp://arxiv.org/abs/astro-ph/9905149
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/18394
dc.subjectAstrophysics
dc.titleCluster Formation and the ISM
dc.typetext

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