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.

Programme(s)

• FP2-SCIENCE - Programme plan (EEC) to stimulate the international cooperation and interchange needed by European research scientists (SCIENCE), 1988-1992

Funding Scheme

CSC - Cost-sharing contracts

Coordinator

University of Kent at Canterbury

Address

CT2 7NT Canterbury
United Kingdom