Abstract
We present an analysis of the data from our Swedish-ESO Submillimetre Telescope molecular line survey in the 1.3 mm band of the N, M, and NW positions in the Sgr B2 molecular cloud. The line emissions from 42 molecular species, and some of their isotopomers, were analyzed assuming a single temperature and a homogeneous source. In cases where a source size much smaller than the antenna beam (23
Original language | English |
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Pages (from-to) | 213-243 |
Number of pages | 31 |
Journal | Astrophysical Journal Supplement |
Volume | 128 |
Issue number | 1 |
Publication status | Published - May 2000 |
ASJC Scopus subject areas
- Space and Planetary Science