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

Dignant

outset

运动性

痛得哭了

Recess

低三下四之人

Changes in Interstellar Atomic Abundances from the Galactic Plane to the Halo,not seem to change appreciably. A likely explanation for the apparent increase of iron is the partial sputtering of material off the surfaces of dust grains by interstellar shocks. Another possibility might be that the ejecta from type I supernovae enrich the low density medium in the halo with iron.

Instinctive

苦涩

enumaerate

On the Analysis of Motions Perpendicular to the Galactic Plane,one has succeeded in deriving a valid curve of the acceleration ..; typically the curve turns over in a way that implies negative densities at some distance from the galactic plane. What I would like to do in this brief note is to suggest some possible reasons for this difficulty--specifically, that the types of stars used have been unsuitable.

束以马具

0067-0057 d at Penticton in June 1981. Leo Blitz (now at the University of Maryland) and I decided that there was a need, and agreed that we would organize one in Vancouver in the Spring of 1982. The purpose of the workshop was to have an intensive exchange of ideas between some of the most active workers in