MOLECULAR ABUNDANCES IN THE MAGELLANIC CLOUDS .2. DEUTERATED SPECIES IN THE LMC

Citation
Yn. Chin et al., MOLECULAR ABUNDANCES IN THE MAGELLANIC CLOUDS .2. DEUTERATED SPECIES IN THE LMC, Astronomy and astrophysics, 312(3), 1996, pp. 33-36
Citations number
19
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00046361
Volume
312
Issue
3
Year of publication
1996
Pages
33 - 36
Database
ISI
SICI code
0004-6361(1996)312:3<33:MAITMC>2.0.ZU;2-Z
Abstract
The first definite discoveries of extragalactic deuterium are reported . DCO+ has been detected in three and DCN has been measured in one sta r-forming region of the Large Magellanic Cloud (LMC). While the HCO+/D CO+ abundance ratios are found to be 19 +/- 3, 24 +/- 4, and 67 +/- 18 for N113, N44BC and N159HW, respectively, a HCN/DCN abundance ratio o f 23 +/- 5 is obtained for N113. These results are consistent with a g as temperature of about 20 K and a D/H ratio of about 1.5 x 10(-5), co nsistent with that observed in the Galaxy. If the cloud temperature is closer to 30 K, then a D/H ratio is required to be up to an order of magnitude larger. Because this ratio provides a lower limit to the pri mordial D/H ratio, it indicates that the baryon mass density alone is unable to close the universe.