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Evidence for Protostellar Wind-Cloud Interactions

Published online by Cambridge University Press:  12 April 2016

Alexander L. Rudolph
Alexander L. Rudolph*
Affiliation:
NASA/Ames Research Center, Mail Stop 245-6, Moffett Field, Calif. 94035 U.S.A.

Abstract

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Recent molecular line observations of HH flows (HH objects and optical jets) have revealed abundant evidence of interactions between protostellar winds and the surrounding molecular clouds. HCO+ observations taken with the BIMA Array have traced out the distribution of both stationary and high-velocity gas near the protostellar objects HH 7-11, L1551, and HH 34.

Type
3. Astronomical Results and Prospects
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 195 - 198
Copyright
Copyright © Astronomical Society of the Pacific 1994

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