Molecular abundances in the Magellanic Clouds .2. Deuterated species in the LMC


Autoria(s): Chin, Y.N.; Henkel, C.; Millar, TJ; Whiteoak, J.B.; Mauersberger, R.
Data(s)

1996

Resumo

The first definite discoveries of extragalactic deuterium are reported. DCO+ has been detected in three and DCN has been measured in one star-forming region of the Large Magellanic Cloud (LMC). While the HCO+/DCO+ abundance ratios are found to be 19 +/- 3, 24 +/- 4, and 67 +/- 18 for N113, N44BC and N159HW, respectively, a HCN/DCN abundance ratio of 23 +/- 5 is obtained for N113. These results are consistent with a gas temperature of about 20 K and a D/H ratio of about 1.5 x 10(-5), consistent 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 primordial D/H ratio, it indicates that the baryon mass density alone is unable to close the universe.

Identificador

http://pure.qub.ac.uk/portal/en/publications/molecular-abundances-in-the-magellanic-clouds-2-deuterated-species-in-the-lmc(48851edf-cabd-490a-b826-7ecf6607a42b).html

Idioma(s)

eng

Direitos

info:eu-repo/semantics/restrictedAccess

Fonte

Chin , Y N , Henkel , C , Millar , T J , Whiteoak , J B & Mauersberger , R 1996 , ' Molecular abundances in the Magellanic Clouds .2. Deuterated species in the LMC ' Astronomy and Astrophysics , vol 312 , pp. L33-L36 .

Tipo

article