Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4133
Title: RS CVn-type variables. I - Photometry of HR 1099
Authors: Parthasarathy, M
Raveendran, A. V
Mekkaden, M. V
Keywords: Binary Stars;Light Curve;Stellar Spectrophotometry;Variable Stars;Emission Spectra;H Alpha Line;Stellar Luminosity
Issue Date: Jan-1981
Publisher: D. Reidel Publishing Co.
Citation: Astrophysics and Space Science, Vol. 74, No. 1, pp. 87 - 96
Abstract: Photometric observation of HR 1099 inV andB obtained on 18 nights between January and March 1977 is presented. The amplitude of the asymmetric light curve is found to be 0m.10±0m.004 both inV andB. On three occasions—namely, JD 2443164. 17, JD 2443176. 14 and JD 2443177.12—the star brightened by 0m.05. Four H spectrograms at 42 Å mm–1 dispersion were obtained during October–November 1978. The profile and equivalent width of H of 14 November, 1978 suggest a probable major outburst. Analysis of all available photometry shows that (1) the amplitude and shape of the light curve change in a few orbital periods, (2) the phase of the minimum light migrated towards decreasing orbital phase during the interval JD 2442720 to JD 2443000 and from JD 2443200, there is almost a linear increase of the phase of the minimum light and (3) the phase of the light minimum sometimes shows to and fro behaviour suggesting the migration of the wave is not taking place smoothly.
URI: http://hdl.handle.net/2248/4133
ISSN: 0004-640X
???metadata.dc.relation.uri???: http://adsabs.harvard.edu/abs/1981Ap%26SS..74...87P
http://dx.doi.org/10.1007/BF00642084
Appears in Collections:IIAP Publications

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