The Origin of Stars and Planetary Systems 1999
DOI: 10.1007/978-94-011-4509-1_15
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Massive Star Formation

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Cited by 81 publications
(31 citation statements)
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“…When Herschel photometry is included,Ṁ env /M increases to (2,3,2,4) × 10 −4 yr −1 . The higher infall rates are in agreement with previous outflow studies of massive protostars (Churchwell 1999). The implied ages of <10 4 yr further strengthen the assertion that Herschel probes the very youngest sources.…”
Section: Modeled Physical Propertiessupporting
confidence: 90%
“…When Herschel photometry is included,Ṁ env /M increases to (2,3,2,4) × 10 −4 yr −1 . The higher infall rates are in agreement with previous outflow studies of massive protostars (Churchwell 1999). The implied ages of <10 4 yr further strengthen the assertion that Herschel probes the very youngest sources.…”
Section: Modeled Physical Propertiessupporting
confidence: 90%
“…In particular, Churchwell (1997) pointed out that the mass flux in such outflows is enormous, and it is unclear that entrainment of ambient material by the outflow can proceed quickly enough to supply it.…”
Section: Introductionmentioning
confidence: 99%
“…This mass accretion rate, first used by Behrend & Maeder (2001), was inspired by the observational correlation between mass outflows and bolometric luminosities in ultra-compact HII regions (Churchwell 1999;Henning et al 2000) and from a fit with observed Herbig Ae/Be stars (Behrend & Maeder 2001). Because the luminosity of the star changes during accretion, the mass accretion rate is time dependent, and except for very early in the pre-MS evolution, it increases with the age.…”
Section: Relevance Of the Internal Rotational Profilementioning
confidence: 99%