Titlebook: Kinematics, Dynamics and Structure of the Milky Way; Proceedings of a Wor W. L. H. Shuter Conference proceedings 1983 D. Reidel Publishing

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Conference proceedings 1983y of the points raised have been in the publications, and it seems pointless to reproduce it incorporated here. Leo and I would like to thank the many people who helped to make the meeting a success: at UBC) and Frank J. Kerr (Provost of MPSE C.V. Finnegan (Dean of Science at the University of Maryl

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Gamma Radiation as a Tracer of the Local Interstellar Gas,y in gamma rays of energy greater than 50 MeV. The Milky Way is completely covered (Mayer-Hasselwander et al. 1982) and at all longitudes the survey is extended to medium latitude regions at |b|≲20° or at some selected regions even further.

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The Large-Scale Structure of Atomic Hydrogen,. The Parkes 18m and Hat Creek 26m surveys have been used to study the distribution of HI in the outer Galaxy based on a circular rotation model. The surface density distribution is discussed, and also the warping and the thickness of the HI layer. The total mass of HI in the Galaxy is found to be 4.8 × 10. M..

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Local Galactic Structure and Velocity Field,The information contained in the local stellar velocity field is discussed. The local expansion, also reveiled by the interstellar gas, is interpreted in terms of a scenario where giant clouds are formed in galactic shocks, give birth to stars and subsequently expand.

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