Outflows and jets from massive star-forming clusters

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dc.creatorBeuther, H.
dc.date2004-04-28
dc.date.accessioned2026-07-07T02:13:01Z
dc.date.available2026-07-07T02:13:01Z
dc.descriptionStudying outflows from young massive star-forming clusters allows one to deduce physical processes that lead to the formation of the most massive stars. I will review the current state of high-spatial-resolution interferometric (sub-)mm studies of massive molecular outflows and their implications for high-mass star formation. A possible evolutionary scenario for massive outflows with highly collimated structures at the very beginning and more wind-like outflows at later stages will be outlined.
dc.description8 pages, 4 figures, conference proceedings (invited talk) of the "X-ray and Radio Connections" meeting in Santa Fe in February 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0404563
dc.identifierhttp://arxiv.org/abs/astro-ph/0404563
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7669
dc.subjectAstrophysics
dc.titleOutflows and jets from massive star-forming clusters
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