Add to ORKGNew BVRI light curves of the eclipsing binary BG Peg were obtained and analysed using the Wilson-Devinney code. The observations (102 hours during a span of 108 days) were collected to perform an accurate frequency analysis of the pulsations of the primary component of the system, which is of δ Sct type. Three pulsation frequencies were identified in that star
This work presents an extensive analysis of the properties of three southern semi-detached eclipsing...
International audienceWe present a preliminary spectroscopic analysis of the binary system V577Oph, ...
WOS: 000349503400011The eclipsing binary OO Peg consist of two late-A type stars in circular orbit w...
New BVRI light curves of the eclipsing binary BG Peg were obtained and analysed using the Wilson-Dev...
WOS: 000185676200023New photometric observations of the Algol-type binary system AB Cassiopeiae were...
We present CCD photometric results of the eclipsing binary Y Cam, whose primary component has been k...
V453 Cyg is an eclipsing binary containing 14 and 11 M⊙ stars in an eccentric short-period orbit. We...
Stars that are both pulsating and eclipsing offer an important opportunity to better understand many...
WX Eri is an eclipsing binary system for which one component was reported to show δ Scuti type puls...
We present the results of a systematic search for pulsating components in Algol-type eclipsing binar...
Initial results from a photometric survey of stars selected from the list of eclips-ing binaries tha...
This work presents an extensive analysis of the properties of three southern semi-detached eclipsing...
We present a preliminary analysis of time series photometry on the pulsating subdwarf B star PG1336-...
Abstract We present a long-term time-resolved photometry of the short-period eclipsing binary IU Per...
Context. This research paper contains light curve modelling, spectroscopy, and detailed asteroseismi...
This work presents an extensive analysis of the properties of three southern semi-detached eclipsing...
International audienceWe present a preliminary spectroscopic analysis of the binary system V577Oph, ...
WOS: 000349503400011The eclipsing binary OO Peg consist of two late-A type stars in circular orbit w...
New BVRI light curves of the eclipsing binary BG Peg were obtained and analysed using the Wilson-Dev...
WOS: 000185676200023New photometric observations of the Algol-type binary system AB Cassiopeiae were...
We present CCD photometric results of the eclipsing binary Y Cam, whose primary component has been k...
V453 Cyg is an eclipsing binary containing 14 and 11 M⊙ stars in an eccentric short-period orbit. We...
Stars that are both pulsating and eclipsing offer an important opportunity to better understand many...
WX Eri is an eclipsing binary system for which one component was reported to show δ Scuti type puls...
We present the results of a systematic search for pulsating components in Algol-type eclipsing binar...
Initial results from a photometric survey of stars selected from the list of eclips-ing binaries tha...
This work presents an extensive analysis of the properties of three southern semi-detached eclipsing...
We present a preliminary analysis of time series photometry on the pulsating subdwarf B star PG1336-...
Abstract We present a long-term time-resolved photometry of the short-period eclipsing binary IU Per...
Context. This research paper contains light curve modelling, spectroscopy, and detailed asteroseismi...
This work presents an extensive analysis of the properties of three southern semi-detached eclipsing...
International audienceWe present a preliminary spectroscopic analysis of the binary system V577Oph, ...
WOS: 000349503400011The eclipsing binary OO Peg consist of two late-A type stars in circular orbit w...