The Morphology and Dynamics within 200 AU of the High-Mass Protostar, Source~I in Orion BN/KL

Details The Morphology and Dynamics within 200 AU of the High-Mass Protostar, Source~I in Orion BN/KL The Morphology and Dynamics within 200 AU of the High-Mass Protostar, Source~I in Orion BN/KL

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..357c&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

Astronomy and Astrophysics

Astronomy

3

Scientific paper

High-resolution imaging of the SiO v=0 and v=1, J=1-0 masers associated with the high-mass protostar, Source I in Orion BN/KL, reveals the dynamics of dense circumstellar gas at radii of a few 100 AU. The masers appear to trace the edges of a collimated, high-velocity, conical flow, and a much more wide-angle, low-velocity flow. These two flow components may indicate multiple phases of mass-loss from Source I.

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