The predicted 1s2-1s6p H/-/ auto-ionization resonance observed as a diffuse interstellar line at 7581 A

Details The predicted 1s2-1s6p H/-/ auto-ionization resonance observed as a diffuse interstellar line at 7581 A The predicted 1s2-1s6p H/-/ auto-ionization resonance observed as a diffuse interstellar line at 7581 A

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..319g&link_type=abstract

Astrophysics and Space Science, vol. 72, no. 2, Oct. 1980, p. 319-322.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Spectroscopy, Autoionization, Infrared Spectra, Line Spectra, Stellar Spectra, B Stars, Interstellar Extinction, Near Infrared Radiation, O Stars, Spectral Line Width

Scientific paper

The 1s2-ls6p H auto-ionization resonance has been observed as a diffuse interstellar line in several highly reddened 0 and B stars. The identification based on its wavelength has been confirmed by its equivalent width in HD 183143. The addition of the 1s2-Isnp diffuse-line series raises the total H - oscillator strength of absorption to a value close to 2

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