Parsec-Scale Outflows from Intermediate-Mass Stars

Details Parsec-Scale Outflows from Intermediate-Mass Stars Parsec-Scale Outflows from Intermediate-Mass Stars

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..141m&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Stars: Formation, Ism: Jets And Outflows, Stars: Pre-Main Sequence

Scientific paper

While there are many large-scale outflows which are known to be driven by low-mass sources, there are few such outflows associated with higher mass sources. In this survey, parsec-scale outflows were found from five intermediate-mass sources. These show similar length, morphology, dynamical timescales, and collimation as parsec-scale outflows from low-mass sources. Many of these outflows also appear to have blown out of the parent cloud, suggesting that the total length of the outflow is greater than what is optically observable.

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