Our photometric monitoring of CH Cyg revealed a gradual increase of its brightness in U from 2010. More recent observations, made during 2014–2015 suggest that CH Cyg entered a new active phase. Monitoring for rapid variability demonstrated unambiguous connection between appearance of pronounced rapid variations and the level of the overall brightness in U, i.e. the activity of CH Cyg
We present a preliminary analysis of our five-years observation campaign of the B[e] stellar system ...
We present V light curves of P Cygni from JD 2446200-9300 (1985-1993). Inspection of the light curv...
Context. V2492 Cyg is a young pre-main sequence star presenting repetitive brightness variations of ...
We analyse a light curve of the symbiotic star BF Cyg, covering 114 years of its photometric history...
We present the results of new multicolor photometry of the chromospherically active binary CG Cyg ac...
In order to help answering the question generally posed for symbiotic stars: are the apparently ina...
We present recent photometric observations of Z And, BF Cyg, and AX Per made in the standard Johnson...
International audienceWe have detected asymmetry in the symbiotic star CH Cyg through the measuremen...
We report new photometry of CG Cyg from 1998–2002. We also analyze published photometry collected si...
We present new photometric data for seven high-amplitude δ Scuti stars. The observations were acquir...
Context. CH Cyg is one of the most studied symbiotic stars. Its properties, however, are still not w...
DM Cyg, a fundamental mode RRab star, was observed in the 2007 and 2008 seasons in the framework of ...
We are intensively monitoring the current outburst on BF Cyg, both spectroscopically (high and low r...
Aim. We aimed to perform the analysis of the long-term variability and precession of the orbital inc...
Context. The outburst of the symbiotic recurrent nova V407 Cyg in 2010 has been studied by numerous ...
We present a preliminary analysis of our five-years observation campaign of the B[e] stellar system ...
We present V light curves of P Cygni from JD 2446200-9300 (1985-1993). Inspection of the light curv...
Context. V2492 Cyg is a young pre-main sequence star presenting repetitive brightness variations of ...
We analyse a light curve of the symbiotic star BF Cyg, covering 114 years of its photometric history...
We present the results of new multicolor photometry of the chromospherically active binary CG Cyg ac...
In order to help answering the question generally posed for symbiotic stars: are the apparently ina...
We present recent photometric observations of Z And, BF Cyg, and AX Per made in the standard Johnson...
International audienceWe have detected asymmetry in the symbiotic star CH Cyg through the measuremen...
We report new photometry of CG Cyg from 1998–2002. We also analyze published photometry collected si...
We present new photometric data for seven high-amplitude δ Scuti stars. The observations were acquir...
Context. CH Cyg is one of the most studied symbiotic stars. Its properties, however, are still not w...
DM Cyg, a fundamental mode RRab star, was observed in the 2007 and 2008 seasons in the framework of ...
We are intensively monitoring the current outburst on BF Cyg, both spectroscopically (high and low r...
Aim. We aimed to perform the analysis of the long-term variability and precession of the orbital inc...
Context. The outburst of the symbiotic recurrent nova V407 Cyg in 2010 has been studied by numerous ...
We present a preliminary analysis of our five-years observation campaign of the B[e] stellar system ...
We present V light curves of P Cygni from JD 2446200-9300 (1985-1993). Inspection of the light curv...
Context. V2492 Cyg is a young pre-main sequence star presenting repetitive brightness variations of ...