We have obtained 551 new V and R observations of the RR Lyrae star DR Andromedae. Our data set is consistent with a primary period of 0.563118 days; however, the light curve of DR And cannot be well described by a single period. We conclude that DR And demonstrates the Blazhko effect with a Blazhko period of approximately 57.5 days
The cause of the Blazhko effect, the long-term modulation of the light and radial velocity curves of...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
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 462 new V and R observations of the RR Lyrae star GV Andromedae. Our data set is ...
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...
With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rath...
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. Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003-2004, covering mor...
We present the first results of our analyses of selected RR Lyrae stars for which data have been obt...
With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rath...
The cause of the Blazhko effect, the long-term modulation of the light and radial velocity curves of...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
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 462 new V and R observations of the RR Lyrae star GV Andromedae. Our data set is ...
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...
With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rath...
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. Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003-2004, covering mor...
We present the first results of our analyses of selected RR Lyrae stars for which data have been obt...
With increasingly accurate data on RR Lyrae stars we find that the Blazhko effect may be a rule rath...
The cause of the Blazhko effect, the long-term modulation of the light and radial velocity curves of...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...
Aims.Extensive photometry of RR Lyr was obtained over a 421-day interval in 2003–2004, covering mor...