Time-series data taken with the Hubble Space Telescope of three fields covering the central part of the globular cluster M22 have been analyzed in search of variable objects. We report identification of 11 periodic variables of which 8 are new discoveries. The sample includes 5 certain contact binaries as well as 1 SX Phe star. Two objects with periods longer than 1 day are preliminarily classified as either spotted variables of BY Dra type or ellipsoidal variables. The most unusual of the identified variables, M22_V11, has I_C=19.9 and is located far to the red of the main sequence in the cluster color-magnitude diagram. It shows variability with a period as short as P=0.066 days or alternatively with P=0.132 days. We propose that it may b...
The $\rm 13.6\, \times\, 13.6\ arcmin^{2}$ field including the central part of the globular cluster...
Abstract. Three elds located close to the center of the globular cluster! Cen were surveyed in a sea...
Aims. We aim to obtain time-series photometry of the very crowded central regions of Galactic globul...
Results of a search for variable stars in the central region of the Oosterhoff II type globular cl...
We describe here the results of a photometric time-sequence survey of the globular cluster M3 (NGC 5...
Using an image subtraction method we have searched for variable stars in the globular cluster M14. W...
We report on the results of a long time photometric monitoring of the two metal-poor Galactic globul...
Context. We present a new search for variable stars in the Galactic globular cluster M 28 (NGC 6626)...
Time-series data taken with the Hubble Space Telescope of a field six core radii (5') from the cente...
Time-series data taken with the Hubble Space Telescope of a field six core radii (~5') from the cent...
A 67" x 104" area of the metal-rich globular cluster M71 was searched for variable stars using 73 CC...
Three fields covering the central part of the globular cluster ω Cen were surveyed in a search for ...
The central part of the globular cluster NGC 288 was surveyed in a search for short-period variable...
Three fields located close to the center of the globular cluster ω Cen were surveyed in a search fo...
Nineteen variable stars with periods greater than one day were observed in six globular clusters. Th...
The $\rm 13.6\, \times\, 13.6\ arcmin^{2}$ field including the central part of the globular cluster...
Abstract. Three elds located close to the center of the globular cluster! Cen were surveyed in a sea...
Aims. We aim to obtain time-series photometry of the very crowded central regions of Galactic globul...
Results of a search for variable stars in the central region of the Oosterhoff II type globular cl...
We describe here the results of a photometric time-sequence survey of the globular cluster M3 (NGC 5...
Using an image subtraction method we have searched for variable stars in the globular cluster M14. W...
We report on the results of a long time photometric monitoring of the two metal-poor Galactic globul...
Context. We present a new search for variable stars in the Galactic globular cluster M 28 (NGC 6626)...
Time-series data taken with the Hubble Space Telescope of a field six core radii (5') from the cente...
Time-series data taken with the Hubble Space Telescope of a field six core radii (~5') from the cent...
A 67" x 104" area of the metal-rich globular cluster M71 was searched for variable stars using 73 CC...
Three fields covering the central part of the globular cluster ω Cen were surveyed in a search for ...
The central part of the globular cluster NGC 288 was surveyed in a search for short-period variable...
Three fields located close to the center of the globular cluster ω Cen were surveyed in a search fo...
Nineteen variable stars with periods greater than one day were observed in six globular clusters. Th...
The $\rm 13.6\, \times\, 13.6\ arcmin^{2}$ field including the central part of the globular cluster...
Abstract. Three elds located close to the center of the globular cluster! Cen were surveyed in a sea...
Aims. We aim to obtain time-series photometry of the very crowded central regions of Galactic globul...