The far UV spectrum of the Be star 88 Herculis

Details The far UV spectrum of the Be star 88 Herculis The far UV spectrum of the Be star 88 Herculis

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...72..497d&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 72, no. 3, March 1988, p. 497-504.

Astronomy and Astrophysics

Astrophysics

3

B Stars, Stellar Spectra, Ultraviolet Spectra, Far Ultraviolet Radiation, Identifying, Iue, Line Spectra

Scientific paper

A high-resolution FUV spectrum of 88 Her, obtained with the IUE short-wavelength primary instrument on May 23, 1984, is analyzed. Line identifications for the 110-210-nm range, determined on the basis of the multiplet tables of Moore (1968) and Kelly and Palumbo (1979) are presented in a table, and a list of unidentified lines is also provided. The spectrum is characterized by crowded shell absorption lines, with Fe II and Ni II dominant.

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