Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.158..123g&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 158, no. 1, Aug. 1989, p. 123-133.
Astronomy and Astrophysics
Astronomy
2
Accretion Disks, Stellar Spectra, Stellar Temperature, Symbiotic Stars, Triple Stars, Ultraviolet Astronomy, Emission Spectra, Line Spectra, Nebulae, White Dwarf Stars
Scientific paper
The conditions of the excitation of ultraviolet emission lines in symbiotic stars-triple systems with white dwarf and nebular clouds are examined. A new method is suggested for the determination of effective temperature of the accretion disk around of white dwarf, which is based on the balance between the summary intensities of ultraviolet emission lines, escaped by nebular cloud, and a definite part of the energy of blackbody radiation of accretion disk in the region shorter from the some wavelength. The results of the application of this method in relation to the five symbiotic triple-star systems are presented.
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