Physical State of Interstellar Atoms

Details Physical State of Interstellar Atoms Physical State of Interstellar Atoms

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974rspsa.340..447y&link_type=abstract

Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences, Volume 340, Issue 1623, pp. 447-455

Physics

1

Scientific paper

A brief survey is given of the physical conditions along the lines of sight to reddened and unreddened stars, as determined from Copernicus observation of interstellar lines between 95 and 300 nm. Differences in ionization structure and density between clouds and the local intercloud medium are discussed. Some new data for β Centauri is used to supplement the previously available data.

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