Neutral atomic absorption lines and far-UV extinction: Possible implications for depletions and grain parameters

Details Neutral atomic absorption lines and far-UV extinction: Possible implications for depletions and grain parameters Neutral atomic absorption lines and far-UV extinction: Possible implications for depletions and grain parameters

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990nascp3084...42w&link_type=abstract

In NASA, Ames Research Center, The Interstellar Medium in External Galaxies: Summaries of Contributed Papers p 42-44 (SEE N91-14

Physics

Absorption Spectra, Depletion, Extinction, Far Ultraviolet Radiation, Ionization, Line Spectra, Magellanic Clouds, Neutral Atoms, Abundance, Ratios, Variations

Scientific paper

Researchers examine nine lines of sight within the Galaxy and one in the Large Magellanic Cloud (LMC) for which data on both neutral atomic absorption lines (Snow 1984; White 1986; Welty, Hobbs, and York 1989) and far UV extinction (Bless and Savage 1972; Jenkins, Savage, and Spitzer 1986) are available, in order to test the assumption that variations in gamma/alpha will cancel in taking ratios of the ionization balance equation, and to try to determine to what extent that assumption has affected the aforementioned studies of depletions and grain properties.

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