Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...319l..21h&link_type=abstract
Astronomy and Astrophysics, v.319, p.L21-L24
Astronomy and Astrophysics
Astrophysics
5
Ism: Molecules, Galaxies: Abundances, Galaxies: Ism, Magellanic Clouds, Radio Lines: Galaxies, Radio Lines: Ism
Scientific paper
We report on the detection of DCO^+^ and, tentatively, DCN in their rotational J=2-1 transitions towards the N159 region in the Large Magellanic Cloud (LMC). These detections of deuterated molecules in an extragalactic source complement those already published by Chin et al. (1996). The resulting estimate of the HCO^+^/DCO^+^ abundance ratio is 120_-60_^+60^ (total 2σ uncertainties). Assuming a Galactic D/H ratio for the LMC leads to an estimate of the kinetic temperature of the molecular gas and an upper limit to the fractional electron abundance of 10-27K and a few x10^-5^, respectively. The temperature estimate is in accordance with excitation calculations using a number of other molecules. The HCO^+^/DCO^+^ abundance ratio in N159 is a factor of a few higher than in cores of Galactic molecular clouds. This is probably due to a somewhat higher gas temperature and possibly a considerably higher electron abundance in N159. The estimated HCN/DCN abundance ratio is 60_-35_^+50^ (total 2σ uncertainties).
Heikkilä Arto
Johansson Lars E. B.
Olofsson Hans
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