Submillimeter Dust Continuum Studies of Low and High Mass Star Formation

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dc.creatorShirley, Yancy L.
dc.creatorMueller, Kaisa E.
dc.creatorYoung, Chadwick H.
dc.creatorEvans II, Neal J.
dc.date2002-05-30
dc.date.accessioned2026-07-07T10:31:16Z
dc.date.available2026-07-07T10:31:16Z
dc.descriptionStudying the physical environments of low mass and high mass cores using dust continuum emission provides important observational constraints on theoretical models of star formation. The motivation and procedure for modeling dust continuum emission is reviewed and the results of recent surveys towards low mass and high mass star forming regions are compared.
dc.description5 pages, 3 figures. To appear in Galactic Star Formation Across the Stellar Mass Spectrum, ASP conf. series, ed. James M. De Buizer
dc.identifierhttps://arxiv.org/abs/astro-ph/0205519
dc.identifierhttp://arxiv.org/abs/astro-ph/0205519
dc.identifierASPConf.Ser.287:298-304,2003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178353
dc.subjectAstrophysics
dc.titleSubmillimeter Dust Continuum Studies of Low and High Mass Star Formation
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