The ultraviolet behavior of Z Andromedae during quiescence and outburst

Details The ultraviolet behavior of Z Andromedae during quiescence and outburst The ultraviolet behavior of Z Andromedae during quiescence and outburst

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..225f&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 225-227 (SEE N86-20287 10-93)

Computer Science

2

Andromeda Constellation, Stellar Spectra, Symbiotic Stars, Ultraviolet Spectra, Iue, Periodic Variations, Stellar Models

Scientific paper

The UV variability of Z Andromedae symbiotic stars was monitored by IUE. Results show that the observed UV-near Ir energy distribution can be accounted for by three components: a latetype giant star, responsible for the observed flux in the near IR; a compact object providing the observed spectrum in the far-UV; and an extended nebular region giving rise to gas recombination continuum and emission lines.

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