Mass loss rates from protostars and OI(63 micron) shock luminosities

Details Mass loss rates from protostars and OI(63 micron) shock luminosities Mass loss rates from protostars and OI(63 micron) shock luminosities

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icar...61...36h&link_type=abstract

(Conference on Protostars and Planets II, Tucson, AZ, Jan. 4-7, 1984) Icarus (ISSN 0019-1035), vol. 61, Jan. 1985, p. 36-39.

Physics

43

Mass Flow Rate, Oxygen Spectra, Protostars, Shock Wave Luminescence, Stellar Mass Ejection, Emission Spectra, Shock Wave Propagation, Stellar Luminosity, Stellar Winds

Scientific paper

The high-velocity ejection of material from protostars results in a wind shock which may be observable in O I (63 μm) emission. It is shown that for a wide range of conditions, the O I (63 μm) luminosity is proportional to the mass loss rate from the protostar. Application is made to shock O I (63 μm) emission observed around IRc 2 in the BN-KL region of Orion.

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