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Content archived on 2024-04-16

Millimeter and sub-millimeter wavelength studies of star formation regions


Studies conducted are as follows:
methyl cyanide in Orion-KL;
ammonia (1,1) and (2,2) emission from recently discovered candidate protostellar objects;
mapping G43.3 in various near infrared bands;
a 330-360 GHz spectral line survey in G34.3;
the statistical equilibrium modelling program has been altered to allow modelling of the interferometric maps of methyl cyanide (J=6-5) of G34.3 made with the Nobeyama millimetre array;
MERLIN 5 GHz continuum mapping of G34.3.


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University of Kent at Canterbury
EU contribution
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CT2 7NT Canterbury
United Kingdom

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