The contribution of disks and envelopes to the millimeter continuum emission from very young low-mass stars

We investigate the question of disk formation during the protostar phase. We model the dust continuum emission from the dense cloud core using the cloud-collapse models of Terebey et al. (1984) and show that dust emission from the dense core is important when measured with large single-dish telescop...

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Veröffentlicht in:The Astrophysical journal 1993-09, Vol.414 (2), p.759-772
Hauptverfasser: Terebey, S., Chandler, C. J., Andre, P.
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Sprache:eng
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