Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4100
Title: Spot activity in the RS CVn binary HR 1099
Authors: Mekkaden, M. V
Raveendran, A. V
Mohin, S
Keywords: Astronomical Photometry;Binary Stars;Starspots;Ubv Spectra;Light Curve;UBV Photometry;RS CVn Variables;Spot Activity
Issue Date: Mar-1982
Publisher: Indian Academy of Sciences
Citation: Journal of Astrophysics and Astronomy, Vol. 3, pp. 27 - 38
Abstract: UBV photometry of HR 1099 obtained during the 1979-80 and 1980-81 observing seasons is presented. An analysis of the available data shows that the brightness at the light curve maximum increases as the wave amplitude increases, while the brightness at the light minimum remains almost the same. In terms of the starspot model it implies that there is always a hemisphere of the active component that is nearly 'saturated' with spots and that spots occupy a larger fraction of the stellar surface when the wave amplitude is smaller. The continuous migration attributed to the photometric wave by various authors is far from certain. The amplitude of the wave has a sharp rise followed by slow decay with a period around 5-6 yr. It is found that the two-spot model proposed by Dorren and Guinan (1982) is inadequate to describe all the observed photometric peculiarities of HR 1099.
Description: Open Access
URI: http://hdl.handle.net/2248/4100
ISSN: 0250 - 6335
???metadata.dc.rights???: © Indian Academy of Sciences
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1982JApA....3...27M
http://www.springerlink.com/content/875t3568h0w153r6/
Appears in Collections:IIAP Publications

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