Molecular Gas Around Young Stellar Clusters

Simple item page
dc.creatorRidge, Naomi A.
dc.creatorMegeath, Tom
dc.creatorWilson, T. L.
dc.date2001-10-12
dc.date.accessioned2026-07-07T02:00:48Z
dc.date.available2026-07-07T02:00:48Z
dc.descriptionWe have begun a survey of the molecular gas surrounding 31 young clusters in order to investigate the link between environment and the resulting cluster. We present here a preliminary comparison of two clusters in our sample: GGD12-15 and Mon R2. Since both clusters are located in the MonR2 molecular cloud at a distance of 830 pc, observational biases due to differing sensitivities and angular resolutions are avoided.
dc.description2 pages, 2 figures, uses newpasp.sty. To appear in "Hot Star Workshop III: The Earliest Phases of Massive Star Birth" (ed. P.A. Crowther)
dc.identifierhttps://arxiv.org/abs/astro-ph/0110297
dc.identifierhttp://arxiv.org/abs/astro-ph/0110297
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3531
dc.subjectAstrophysics
dc.titleMolecular Gas Around Young Stellar Clusters
dc.typetext

Files

Collections

arXiv