The All Sky Automated Survey (ASAS) monitors bright stars (8 mag < V < 14 mag) south of declination +28 deg. The ASAS Catalogue of Variable Stars (ACVS) presently contains 50,099 objects; among them are 2212 objects classified as RR Lyrae pulsating variables. We use ASAS photometric V band data to search for multiperiodicity in those stars. We find that 73 of 1435 RRab stars and 49 of 756 RRc stars exhibit the Blazhko effect. We observe a deficiency of RRab Blazhko variables with main pulsation periods greater than 0.65 days. The Blazhko periods of RRc stars exhibit a strongly bimodal distribution. During our study we discovered the Blazhko effect with multiple periods in object ASAS 050747-3351.9 = SU Col. Blazhko periods of 89.3 d and 65....
We have obtained 462 new V and R observations of the RR Lyrae star GV Andromedae. Our data set is ...
We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is ...
To date, about 40 known RR Lyrae stars are located in the Kepler field. The outstandingly high-preci...
The All Sky Automated Survey (ASAS) monitors bright stars (8 < V < 14 mag) south of declinatio...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
We have obtained 615 new V and R observations of the RR Lyrae star FM Per. A period search identif...
We have obtained 615 new V and R observations of the RR Lyrae star FM Per. A period search identif...
We present our analysis of Kepler observations of 29 RR Lyrae stars, based on 138 d of observation. ...
This thesis investigates the characteristics of the Blazhko effect using data from the SuperWASP arc...
We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is ...
We have obtained 462 new V and R observations of the RR Lyrae star GV Andromedae. Our data set is ...
We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is ...
To date, about 40 known RR Lyrae stars are located in the Kepler field. The outstandingly high-preci...
The All Sky Automated Survey (ASAS) monitors bright stars (8 < V < 14 mag) south of declinatio...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Our survey consists of photometric observations of 107 RR Lyrae stars of type RR$\sb{\rm ab}$ and ha...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
Aims. We set out to compile a catalogue of RRab pulsating variables in the SuperWASP archive and ide...
We have obtained 615 new V and R observations of the RR Lyrae star FM Per. A period search identif...
We have obtained 615 new V and R observations of the RR Lyrae star FM Per. A period search identif...
We present our analysis of Kepler observations of 29 RR Lyrae stars, based on 138 d of observation. ...
This thesis investigates the characteristics of the Blazhko effect using data from the SuperWASP arc...
We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is ...
We have obtained 462 new V and R observations of the RR Lyrae star GV Andromedae. Our data set is ...
We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is ...
To date, about 40 known RR Lyrae stars are located in the Kepler field. The outstandingly high-preci...