OH Observations in the Direction of H2O Masers in the Large Magellanic Cloud

Details OH Observations in the Direction of H2O Masers in the Large Magellanic Cloud OH Observations in the Direction of H2O Masers in the Large Magellanic Cloud

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.215..103g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 215, NO.1/JUL01, P. 103, 1985

Astronomy and Astrophysics

Astronomy

9

Scientific paper

1.6-GHz OH observations have been made towards five LMC H II regions that have been associated with H2O maser emission. Circularly polarized maser emission was observed in two cases, 0510-689 and 0540-696B, but not towards 0540-697A (N159), where emission had been previously reported. Weak OH absorption was detected for two regions (0539-691 and 0540-697A) and possibly a third (0540-696). The optical depths are low (around 0.01), providing additional evidence that molecular densities in the LMC are signficantly lower than in our Galaxy.

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