Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-26T16:34:13.018Z Has data issue: false hasContentIssue false
  • English
  • Français

What Have We Learned from SWAS?

Published online by Cambridge University Press:  21 March 2006

Edwin A. Bergin  and
Gary J. Melnick
Edwin A. Bergin
Affiliation:
University of Michigan, Department of Astronomy, 825 Dennison, 500 Church Street, Ann Arbor, MI 48109, USA email: [email protected]
Gary J. Melnick
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA email: [email protected]
Rights & Permissions [Opens in a new window]

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.

The Submillimeter Wave Astronomy Satellite (SWAS) has recently completed 5.5 years of successful operation. Among the legacies of the mission has been a greater understanding of the abundance and spatial distribution of H2O and O2 within molecular clouds. We summarize SWAS results and discuss how the measured low abundance of water vapor and non-detections of molecular oxygen are suggestive of a general lack of atomic oxygen in the dense centers of molecular clouds. We also present a new more comprehensive model for the oxygen chemistry in the interstellar medium.

Keywords

astrobiology — astrochemistry — ISM: molecules — molecular processes — radiative transfer
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S231: Astrochemistry: Recent Successes and Current Challenges , August 2005 , pp. 309 - 318
Copyright
2006 International Astronomical Union