Titlebook: Submillimetre Astronomy; Proceedings of the K Graeme D. Watt,Adrian S. Webster Conference proceedings 1990 Springer Science+Business Media

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Structure and Fragmentation of Quiescent Molecular Cloudsl scale structure of molecular clouds which provides the boundary conditions to the collapse process and second, the physics of the collapse itself. This paper concentrates on some of the questions to be solved in the first category.

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CO J=3→2 Observations of IRC+10216 properties of stellar winds. It is in particular important to evaluate accurately the mass loss rate from this class of stars, as they may play an important role in the replenishment and enrichment of the interstellar medium. The mass loss rate is one of the parameters that goes into radiative tran

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Far-Infrared and Submillimeter Analysis of a Dense Core: Temperature and Density Structure of L1489e Infrared Telescope Facility (IRTF). Using these images we have constructed maps of the temperature and dust density structure in the vicinity of the forming protostar. In brief, the observed structure is consistent with that of a hot (3000 – 6000 K) point source located on the edge of a cold (10 –

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A New Technique for Surface Measurements of Radio Telescopes surface are being carried out. A new holographic technique is currently under developement, which has a number of advantages over existing techniques. This measurement technique is based on the use of a shearing Fourier Transform Spectrometer (Malacara 1978; Steel 1983) to examine the shape of the

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