eclipsing variable stars
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2004 ◽  
Vol 193 ◽  
pp. 279-282
Author(s):  
H. Jin ◽  
S.-L. Kim ◽  
C.-U. Lee ◽  
D.-J. Lee ◽  
K.-S. Kim

AbstractWe present new multiband photometric results for ROTSE-I δ Sct stars and the Fourier decomposition analysis. Our result shows that most of the stars classified as ROTSE-I δ Sct stars seem to be W UMa type eclipsing variable stars.


1991 ◽  
Vol 9 (2) ◽  
pp. 289-290 ◽  
Author(s):  
Kyu-Dong Oh

AbstractWe examine the period variations of ten eclipsing binary stars and from the combined result, attempt to construct a physical explanation for their behaviour.


1987 ◽  
Vol 7 (2) ◽  
pp. 117-118
Author(s):  
Z. Kviz ◽  
A. P. S. Wong

AbstractIt is shown that for the eclipsing variable stars MP Mus and SV Cen a least squares fitting procedure is more accurate when a linear (intensity) rather than a logarithmic (magnitude) scale is used.


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