Starspot Model of RS CVn Type Binary SZ PSC
In: Journal of Astronomy and Space Sciences, Jg. 17 (2000), Heft 2, S. 189-198
Online
academicJournal
Zugriff:
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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Starspot Model of RS CVn Type Binary SZ PSC
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Autor/in / Beteiligte Person: | Young Woon Kang |
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Zeitschrift: | Journal of Astronomy and Space Sciences, Jg. 17 (2000), Heft 2, S. 189-198 |
Veröffentlichung: | The Korean Space Science Society, 2000 |
Medientyp: | academicJournal |
ISSN: | 2093-5587 (print) ; 2093-1409 (print) |
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