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Observations of Absorption by Water Vapor toward Sagittarius B2

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Published 2000 August 16 © 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation D. A. Neufeld et al 2000 ApJ 539 L111 DOI 10.1086/312853

1538-4357/539/2/L111

Abstract

We have observed the 110-101 pure rotational transitions of both H216O and H218O toward Sagittarius B2 using the Submillimeter Wave Astronomy Satellite. The spectra thereby obtained show a complex pattern of absorption and—in the case of H216O—emission, with numerous features covering a wide range of LSR velocities (-130 to 130 km s-1) and representing absorption both in gas associated with Sgr B2 as well as by several components of foreground gas along the line of sight. The ortho-water abundance derived for the absorbing foreground gas is ~6 × 10-7 relative to H2.

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10.1086/312853