A New Analysis of II-Pegasi 1977 Lightcurve
Abstract
The solution of the inverse photometric problem for spotted stars obtained on the basis of the analytical solution of the direct problem is applied to II Peg 1977 light curve. The geometric parameters of the spot configuration so obtained are unambigously determined in contrast to the cases when analysis of the light curve is done on the basis of numerical modelling. A comparison between both methods has been carried out.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- May 1989
- DOI:
- 10.1007/BF00645212
- Bibcode:
- 1989Ap&SS.155..125K
- Keywords:
-
- Astronomical Photometry;
- Light Curve;
- Starspots;
- Angular Resolution;
- Brightness;
- Computational Astrophysics;
- Stellar Temperature;
- Astrophysics