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Detection of Magnetohydrodynamic Shocks in the L1551 Outflow

Barsony, M. and Scoville, N. Z. and Chandler, C. J. (1994) Detection of Magnetohydrodynamic Shocks in the L1551 Outflow. In: Astronomy with Millimeter and Submillimeter Wave Interferometry. IAU Symposium Proceedings Series. No.140. Astronomical Society of Japan , San Francisco, CA, pp. 222-223. ISBN 9780937707784. https://resolver.caltech.edu/CaltechAUTHORS:20181207-130603103

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Abstract

We report the results of CO J=l—+0 mapping of portions of the blue outflow lobe of L1551 with ~ 7” (N-S) × 4” (E-W) resolution, obtained with the 3-element OVRO millimeter array. Comparison of our interferometer mosaic with lower resolution single-dish data shows that we resolve the strongest single-dish emission regions into filamentary structures, such as are characteristic of shock fronts mapped via their near-infrared H2 emission in other outflow sources.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1017/S0252921100019515DOIArticle
ORCID:
AuthorORCID
Scoville, N. Z.0000-0002-0438-3323
Additional Information:© 1994 Astronomical Society of the Pacific.
Series Name:IAU Symposium Proceedings Series
Issue or Number:140
Record Number:CaltechAUTHORS:20181207-130603103
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20181207-130603103
Official Citation:Barsony, M., Scoville, N., & Chandler, C. (1994). Detection of Magnetohydrodynamic Shocks in the L1551 Outflow. International Astronomical Union Colloquium, 140, 222-223. doi:10.1017/S0252921100019515
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:91577
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:07 Dec 2018 21:15
Last Modified:03 Oct 2019 20:36

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