Hostname: page-component-77c89778f8-m8s7h Total loading time: 0 Render date: 2024-07-18T09:28:52.555Z Has data issue: false hasContentIssue false
  • English
  • Français

Interstellar Line Spectra of a Dense Cloud: The VI Cygni Association

Published online by Cambridge University Press:  14 August 2015

Steven P. Souza  and
Barry L. Lutz
Steven P. Souza
Affiliation:
State University of New York at Stony Brook
Barry L. Lutz
Affiliation:
Lowell Observatory, Flagstaff, Arizona

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.

Spectroscopic observations of the dense interstellar cloud which obscures the VI Cygni association have yielded an optical map of the atomic and molecular constituents in a region which may represent a transition between the diffuse and radio clouds. The velocity of the optical components found is consistent with that of a CO cloud seen in front of No. 12.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 261 - 262
Copyright
Copyright © Reidel 1980 

References

Souza, S. P., and Lutz, B. L. (1977). Astrophys. J. 216, L49.Google Scholar
Souza, S. P., and Lutz, B. L. (1979). Astrophys. J. (Lett.) , in press.Google Scholar