Hostname: page-component-745bb68f8f-b95js Total loading time: 0 Render date: 2025-01-13T00:23:14.842Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Giovanardi, C. et al. 1992, ApJ, submittedGoogle Scholar
Lizano, S. et al. 1988, ApJ, 328, 763 Google Scholar
Moriarty-Schieven, G.H., & Snell, R.L. 1988, ApJ, 332, 364 Google Scholar
Reipurth, B. et al. 1986, A&A, 164, 51 Google Scholar
Reipurth, B., & Heathcote, S. 1992, A&A, in pressGoogle Scholar
Rudolph, A. 1992, ApJ (Letters), 397, L111 CrossRefGoogle Scholar
Rudolph, A., & Welch, W.J. 1988, ApJ, 326, L31 Google Scholar
Rudolph, A., & Welch, W.J. 1992, ApJ, 395, 488 Google Scholar
Snell, R.L., and Edwards, S. 1981, ApJ, 251, 103 Google Scholar
Snell, R.L., & Schloerb, F.B. 1985, ApJ, 295, 490 CrossRefGoogle Scholar