The cataclysmic variable AE Aquarii: orbital variability in V band
Abstract
We present 62.7 hours observations of the cataclysmic variable AE Aqr in Johnson V band. These are non-published archive electro-photometric data obtained during the time period 1993 to 1999. We construct the orbital variability in V band and obtain a Fourier fit to the double-wave quiescent light curve. The strongest flares in our data set are in phase interval 0.6 - 0.8. The data can be downloaded from http://www.astro.bas.bg/~rz/DATA/AEAqr.elphot.dat.
- Publication:
-
Bulgarian Astronomical Journal
- Pub Date:
- July 2017
- Bibcode:
- 2017BlgAJ..27...19Z
- Keywords:
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- Stars: novae;
- cataclysmic variables;
- Accretion;
- accretion disks;
- white dwarfs;
- Stars: individual: AE Aqr