The list of 127 eclipsing stars in optical coincidence with star clusters from the SMC is presented. It was prepared using the catalogs of eclipsing systems and star clusters from the SMC based on observations collected during the OGLE-II microlensing project. Location of 12 eclipsing stars in the color-magnitude diagram of clusters allows to exclude their membership. Photometric data of 73 systems support their membership. The remaining 42 objects were found in loose, faint clusters and therefore no conclusive statement about their membership can be made. All presented data are available from the OGLE archive
We present for the first time Washington CT1 photometry for 11 unstudied or poorly studied candidate...
We describe the Difference Image Analysis (DIA) algorithms and software used to analyze four years (...
We report on the discovery and analysis of short-period (0.1 days $< P <$ 5 days), photometrically v...
We present the catalog of clusters found in the area of ~2.4 square degree in the central regions of...
We present the list of potential multiple star clusters from the central part of the SMC. Presented ...
We present Cepheids located in the close neighborhood of star clusters from the Magellanic Clouds. 2...
Five fields located close to the center of the globular cluster NGC $104=47$ Tuc were surveyed in a...
Abstract. Five elds located close to the center of the globular cluster NGC 104 = 47 Tuc were survey...
We present the first edition of a catalog of variable stars found in the Magellanic Clouds using OGL...
We present the fifth part of the OGLE Catalog of Periodic Variable Stars in the Galactic bulge. 574 ...
We present the second part of the OGLE Catalog of Periodic Variable Stars in the Galactic bulge. 800...
Eclipsing binary stars allow the physics of the component stars to be studied. These systems can pro...
Photographic photometry of 20 star clusters and their adjoining fields has been carried out to dete...
We present the BVI photometric maps of the Large Magellanic Cloud. They contain BVI photometry and a...
We present photometric observations of the MACHO-SMC-1 microlensing candidate collected by the OGLE-...
We present for the first time Washington CT1 photometry for 11 unstudied or poorly studied candidate...
We describe the Difference Image Analysis (DIA) algorithms and software used to analyze four years (...
We report on the discovery and analysis of short-period (0.1 days $< P <$ 5 days), photometrically v...
We present the catalog of clusters found in the area of ~2.4 square degree in the central regions of...
We present the list of potential multiple star clusters from the central part of the SMC. Presented ...
We present Cepheids located in the close neighborhood of star clusters from the Magellanic Clouds. 2...
Five fields located close to the center of the globular cluster NGC $104=47$ Tuc were surveyed in a...
Abstract. Five elds located close to the center of the globular cluster NGC 104 = 47 Tuc were survey...
We present the first edition of a catalog of variable stars found in the Magellanic Clouds using OGL...
We present the fifth part of the OGLE Catalog of Periodic Variable Stars in the Galactic bulge. 574 ...
We present the second part of the OGLE Catalog of Periodic Variable Stars in the Galactic bulge. 800...
Eclipsing binary stars allow the physics of the component stars to be studied. These systems can pro...
Photographic photometry of 20 star clusters and their adjoining fields has been carried out to dete...
We present the BVI photometric maps of the Large Magellanic Cloud. They contain BVI photometry and a...
We present photometric observations of the MACHO-SMC-1 microlensing candidate collected by the OGLE-...
We present for the first time Washington CT1 photometry for 11 unstudied or poorly studied candidate...
We describe the Difference Image Analysis (DIA) algorithms and software used to analyze four years (...
We report on the discovery and analysis of short-period (0.1 days $< P <$ 5 days), photometrically v...