Observation of Bowen fluorescence and other phenomena in five symbiotic stars

Details Observation of Bowen fluorescence and other phenomena in five symbiotic stars Observation of Bowen fluorescence and other phenomena in five symbiotic stars

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103..185w&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, Feb. 1991, p. 185-193. Research supported by Unive

Astronomy and Astrophysics

Astronomy

7

Fluorescence, Stellar Spectrophotometry, Symbiotic Stars, Abundance, Interstellar Extinction, Resonance Lines, Stellar Spectra, Ultraviolet Spectra

Scientific paper

Wavelength measurements and line identifications in the 3200-3600 A regions are presented for the symbiotic stars AG Dra, HM Sge, V1016 Cyg, V1329 Cyg, Z And, and R Aqr. The O III lines excited via Bowen's mechanism are analyzed in detail, and a shell model yielding reasonable shell thicknesses and electron densities is described. The Ne/Fe ratio is derived for five of the systems, and spectra in the blue region are briefly described.

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