EVOLUTION OF MASS OUTFLOW IN PROTOSTARS

EVOLUTION OF MASS OUTFLOW IN PROTOSTARS

We have surveyed 84 Class 0, Class I, and flat-spectrum protostars in mid-infrared [Si II], [Fe II], and [S I] line emission, and 11 of these in far-infrared [O I] emission. We use the results to derive their mass. outflow rates, (M) over dot(w). Thereby we observe a strong correlation of (M) over d...

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Bibliographic Details
Main Authors: Watson, Dan M., Calvet, Nuria P., Fischer, William J., Forrest, W. J., Manoj, P., Megeath, S. Thomas, Melnick, Gary J., Najita, Joan, Neufeld, David A., Sheehan, Patrick D., Stutz, Amelia M., Tobin, John J.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
Herbig-Haro objects
ISM: jets and outflows
shock waves
stars: jets
stars: pre-main sequence stars: protostars
Online Access:http://hdl.handle.net/10150/622058
http://arizona.openrepository.com/arizona/handle/10150/622058

Internet

http://hdl.handle.net/10150/622058
http://arizona.openrepository.com/arizona/handle/10150/622058

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