Observations of absorption by water vapor toward Sagittarius B2

被引:35
作者
Neufeld, DA
Ashby, MLN
Bergin, EA
Chin, G
Erickson, NR
Goldsmith, PF
Harwit, M
Howe, JE
Kleiner, SC
Koch, DG
Patten, BM
Plume, R
Schieder, R
Snell, RL
Stauffer, JR
Tolls, V
Wang, Z
Winnewisser, G
Zhang, YF
Melnick, GJ
机构
[1] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA
[5] Cornell Univ, Natl Astron & Ionosphere Ctr, Dept Astron, Ithaca, NY 14853 USA
[6] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[7] Univ Cologne, Inst Phys 1, D-50937 Cologne, Germany
关键词
ISM : abundances; ISM : clouds; ISM : individual (Sagittarius B2); ISM : molecules; radio lines : ISM;
D O I
10.1086/312853
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have observed the 1(10)-->1(01) pure rotational transitions of both (H2O)-O-16 and (H2O)-O-18 toward Sagittarius B2 using the Submillimeter Wave Astronomy Satellite. The spectra thereby obtained show a complex pattern of absorption and - in the case of (H2O)-O-16 - 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 similar to 6 x 10(-7) relative to H-2.
引用
收藏
页码:L111 / L113
页数:3
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