The 1088 A feature toward reddened stars

Details The 1088 A feature toward reddened stars The 1088 A feature toward reddened stars

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...309..306f&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 309, Oct. 1, 1986, p. 306-310. NSF-supported research.

Astronomy and Astrophysics

Astrophysics

14

Interstellar Extinction, Interstellar Matter, Line Spectra, Ultraviolet Spectra, Chlorine, Oao 3, Oscillator Strengths

Scientific paper

An analysis of the interstellar feature near 1088 A in spectra obtained with the Copernicus satellite suggests that neutral chlorine is the absorber. The mean wavelength, as determined from 15 lines of sight, of 1088.052 + or - 0.023 A compares favorably with the chlorine line at 1088.062 A. A strong correlation with Cl I 1347 A indicates an oscillator strength for 1088 A of 0.04. Above a threshold at N(H2) of roughly 10 to the 19th/sq cm, the equivalent width of 1088 A varies approximately with N(H2). The variation with H2 is similar to the variation of Na I and C I with H2.

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