We report on the discovery of 141 further variable stars found in the field of the open cluster NGC 6819. The stars were identified from time-series photometric data obtained on the Isaac Newton Telescope, La Palma, during two observing runs covering the 19 nights between 1999 June 22-30 and 1999 July 22-31. The variables found include 53 eclipsing binaries, of which eight stars appear to be RS CVns, in addition to 70 stars showing spot activity, 13 showing long-period variability and five variables of other types.</p
We have applied the image subtraction method to images of the peculiar, bimodal-horizontal branch g...
We have applied the image subtraction method to images of the peculiar, bimodal-horizontal branch gl...
The Kepler space telescope has proven to be a gold mine for the study of variable stars. Usually, Ke...
We report on the discovery of 141 further variable stars found in the field of the open cluster NGC ...
We report on the discovery of 25 variable stars plus 13 suspected variables found in the field of th...
Aims:This work presents a high-precision variability survey in the field of the old, super metal-ric...
Context. Recent progress in the seismic interpretation of field ß Cep stars has resulted in improvem...
The nearby galaxies IC 1613 and NGC 6822 were observed over four years to detect short period Cephe...
NGC 6231 is a well-studied young open cluster hosting several variable stars. In the field six β Ce...
The results of a recent CCD photometry survey of variables in a 1 field covering the old open clust...
We present results from our survey for planetary transits in the field of the intermediate-age (~2.5...
We report on the progress of a photometric search for planetary transits of stars in the open cluste...
WOS: 000278399000016Context. Recent progress in the seismic interpretation of field beta Cep stars h...
We present results from our survey for planetary transits in the field of the intermediate-age (simi...
We present the first study of the X-ray population of the intermediate-age rich open cluster NGC 681...
We have applied the image subtraction method to images of the peculiar, bimodal-horizontal branch g...
We have applied the image subtraction method to images of the peculiar, bimodal-horizontal branch gl...
The Kepler space telescope has proven to be a gold mine for the study of variable stars. Usually, Ke...
We report on the discovery of 141 further variable stars found in the field of the open cluster NGC ...
We report on the discovery of 25 variable stars plus 13 suspected variables found in the field of th...
Aims:This work presents a high-precision variability survey in the field of the old, super metal-ric...
Context. Recent progress in the seismic interpretation of field ß Cep stars has resulted in improvem...
The nearby galaxies IC 1613 and NGC 6822 were observed over four years to detect short period Cephe...
NGC 6231 is a well-studied young open cluster hosting several variable stars. In the field six β Ce...
The results of a recent CCD photometry survey of variables in a 1 field covering the old open clust...
We present results from our survey for planetary transits in the field of the intermediate-age (~2.5...
We report on the progress of a photometric search for planetary transits of stars in the open cluste...
WOS: 000278399000016Context. Recent progress in the seismic interpretation of field beta Cep stars h...
We present results from our survey for planetary transits in the field of the intermediate-age (simi...
We present the first study of the X-ray population of the intermediate-age rich open cluster NGC 681...
We have applied the image subtraction method to images of the peculiar, bimodal-horizontal branch g...
We have applied the image subtraction method to images of the peculiar, bimodal-horizontal branch gl...
The Kepler space telescope has proven to be a gold mine for the study of variable stars. Usually, Ke...