Starspot Model of RS CVn Type Binary SZ PSC

Details Starspot Model of RS CVn Type Binary SZ PSC Starspot Model of RS CVn Type Binary SZ PSC

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000jass...17..198k&link_type=abstract

Journal of Astronomy and Space Sciences, vol. 17, no. 2, p. 189-198

Astronomy and Astrophysics

Astronomy

Stars, Astellite, Communication

Scientific paper

The emission lines of the ultraviolet region and the light curves of the optical region have been analyzed to investigate the distorted light curves of SZ Psc. The Mg II emission lines of the IUE spectra confirmed that the chromospheric activity of SZ Psc occurs on the K1 IV star. The distorted light curves in the optical region have been analyzed by the spot model where the spots are on the K1 IV star as the result of the chromospheric activity. The complete photometric solution could be deduced for SZ Psc by the good fitness with the spot model.

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