Optical and ultraviolet absorption studies of cool gas in the Milky Way halo

Details Optical and ultraviolet absorption studies of cool gas in the Milky Way halo Optical and ultraviolet absorption studies of cool gas in the Milky Way halo

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990stia...9248389d&link_type=abstract

IAU, Symposium on Interstellar Disk-Halo Connection in Galaxies, 144th, Leiden, Netherlands, June 18-22, 1990, Paper. 9 p.

Physics

Electromagnetic Absorption, Gas Temperature, Halos, Interstellar Gas, Milky Way Galaxy, Ultraviolet Absorption, Hydrogen Atoms, Hydrogen Ions, Interstellar Matter

Scientific paper

This paper focuses on the contributions from absorption techniques to the knowledge of halo gas with temperatures below 10 to the 5th K. The results from observations of the neutral and singly ionized species on the nature of cool gas in the halo, its structure and its kinematics are presented. An overview of past and optical and ultraviolet observational studies of halo gas is included.

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