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High Resolution Observations of Herbig-Haro Flows

Published online by Cambridge University Press:  23 September 2016

B. Reipurth
Affiliation:
1Institute for Astronomy, University of Hawaii, 2680 Woodlawn Dr, Honolulu, HI 96822, USA
S. Andrews
Affiliation:
1Institute for Astronomy, University of Hawaii, 2680 Woodlawn Dr, Honolulu, HI 96822, USA
J. Bally
Affiliation:
2Center for Astrophysics and Space Astronomy, University of Colorado, Boulder, CO 80309, USA
T. L. Beck
Affiliation:
3Gemini, 670 N.A'ohoku Place, Hilo, HI 96720, USA

Abstract

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Observational techniques with high angular and high spectral resolution have become available in recent years and have had a major impact on the study of Herbig-Haro outflows from very young stars. We discuss new results obtained using WFPC2, ACS and STIS onboard the Hubble Space Telescope, as well as spectroscopic data obtained at the Keck telescope and with the Integral Field Unit at the Gemini telescope. We also discuss centimeter radio continuum maps from the Very Large Array and their importance in testing scenarios for the formation of giant Herbig-Haro flows.

Type
Part 7: Jets and Outflows
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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