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| JK | 
|
|
Telescope | Ref. | |
| (GHz) | (K) | ||||
| 1 | 31,2-31,3 | 481.8 | 144.5 | HIFI | a |
| 2 | 20,2-11,1 | 490.6 | 42.9 | HIFI | a |
| 3 | 11,0-10,1 | 509.2 | 22.3 | HIFI | a |
| 4 | 22,0-30,3 | 537.8 | 131.4 | HIFI | a |
| 5 | 21,1-20,2 | 599.9 | 66.4 | HIFI | a |
| 6 | 11,0-11,1 | 80.6 | 42.9 | IRAM 30-m | b |
| 7 | 31,2- 22,1 | 225.9 | 156.7 | IRAM 30-m | c |
| 8 | 21,1-21,2 | 241.6 | 83.6 | SEST | d |
| 9 | 10,1-00,0 | 464.9 | 0.0 | CSO | e |
| 10 | 11,1-00,0 | 893.6 | 0.0 | CSO | f |
Notes. Rows
1 through 5: summary of all the HDO transitions observed in the HIFI
bands 1a and 1b towards Sgr B2(M) (this work). Rows 6 through 9: list
of previously observed HDO features that were used to constrain the
results of our model (see Sect. 3).
References. (a) this work; (b) Belloche et al., in prep; (c) Jacq et al. (1990); (d) Nummelin et al. (1998); (e) M. Gerin, priv. comm.; (f) Comito et al. (2003).
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