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Introduction to the session

Published online by Cambridge University Press:  14 August 2015

Extract

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There has been a great development in the past few years of observational data of various kinds:

  1. (a) HI observations of high resolution and sensitivity (Cohen and Davies, Burton et al., Kerr et al.)

  2. (b) Observations of molecules, in particular high-resolution observations of CO (Burton, Gordon, Bania, Liszt, Solomon et al.)

  3. (c) Infrared and far-infrared

  4. (d) Ionized gas: hydrogen recombination lines, and in particular Nell (with 4″ beam) (Mezger et al., Townes, Wollman et al.)

Type
VI. THE GALACTIC NUCLEUS
Information
Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 323
Copyright
Copyright © Reidel 1979