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 H 2O 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. © 2006 International Astronomical Union.
CITATION STYLE
Bergin, E. A., & Melnick, G. J. (2005). What have we learned from SWAS? Proceedings of the International Astronomical Union, 1(S231), 309–318. https://doi.org/10.1017/S1743921306007307
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