The Bowen mechanism in HZ Herculis

Details The Bowen mechanism in HZ Herculis The Bowen mechanism in HZ Herculis

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...222l..33m&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 222, May 15, 1978, p. L33-L36. NSF-supported research.

Astronomy and Astrophysics

Astronomy

16

Companion Stars, Oxygen Spectra, Pulsars, Stellar Spectra, Ultraviolet Astronomy, X Ray Stars, Binary Stars, Emission Spectra, Fluorescence, Spectral Line Width

Scientific paper

A successful search for ultraviolet O III Bowen emission lines in HZ Her is reported. The observed ratios of Bowen line strengths in HZ Her are compared with those seen in gaseous nebulae. The detection of UV Bowen emission lines in the spectrum of HZ Her is taken as proof that the Bowen fluorescence mechanism is responsible for the 4640-A emission complex previously observed in the spectra of most optical counterparts of X-ray sources.

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