The UV spectrum of the Be star 88 Herculis

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

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.174...49d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 174, no. 1, Dec. 1990, p. 49-90.

Astronomy and Astrophysics

Astrophysics

3

B Stars, Radial Velocity, Stellar Spectra, Ultraviolet Spectra, Absorption Spectra, Abundance, Iue, Metallicity, Resonance Lines, Stellar Envelopes

Scientific paper

A detailed list and analysis is given of line identifications of the UV spectrum of the Be star 88 Her in the wavelength range 1958-3002 A recorded in May 23, 1984 with the IUE. The spectrum is crowded by shell absorption lines, mostly those of singly ionized iron peak elements. The detailed analysis of the radial velocities measured in the whole spectral range 1100-3002 A is also given.

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