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Content archived on 2024-04-16

Millimeter and sub-millimeter wavelength studies of star formation regions

Objective


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.

Topic(s)

Data not available

Call for proposal

Data not available

Coordinator

University of Kent at Canterbury
EU contribution
No data
Address

CT2 7NT Canterbury
United Kingdom

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Total cost
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