Hostname: page-component-6d856f89d9-fb4gq Total loading time: 0 Render date: 2024-07-16T05:46:52.410Z Has data issue: false hasContentIssue false
  • English
  • Français

Mapping Small Scale Structure in Galactic H ɪ with the VLBA

Published online by Cambridge University Press:  12 April 2016

M. D. Faison ,
W. M. Goss  and
P. J. Diamond
M. D. Faison
Affiliation:
University of Wisconsin, Astronomy Department, Madison, WI 53706, U.S.A.
W. M. Goss
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.
P. J. Diamond
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, 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.

We present the first VLBA maps of Galactic H ɪ opacity towards the QSO 3C 138. The maps show significant opacity structure down to angular scales of 20 mas, which implies density structures in the cold neutral medium on physical scales of 10 AU or less

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 289 - 290
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Davis, R.J., Diamond, P.J., & Goss, W.M. 1996. MNRAS, 283, 1105.CrossRefGoogle Scholar
Diamond, P.J., et al. 1989. ApJ, 347, 302.CrossRefGoogle Scholar
Heiles, C. 1996. ApJ, 481, 192–204.Google Scholar