Add to ORKGNew photoelectric observations of the 6th magnitude suspected eclipsing binary system HD 208496 are presented. A Wilson-Devinney light curve solution reveals a detached system with components approaching the terminal age main sequence. The orbital period is suspected to be variable
HIP 7666 is a variable star newly discovered during the Hipparcos mission and classified as of unkno...
Two-colour photoelectric observations of the eclipsing binary AT Pegasi have been carried out at the...
WOS: 000325510600006The BVR photometric light curves of the eclipsing binary BD And were obtained in...
Of the billions of stars which compose a galaxy, a few will be members of the so called eclipsing bi...
Two-colour photoelectric observations of the new eclipsing binary HD 199497 are presented. Our obser...
We present ground-based photoelectric observations of the newly discovered eclipsing binary system V...
We investigate four eclipsing binary systems V508 Cyg, V719 Her, DN Aur and KN Per, selected from Be...
New observations of the eclipsing binary system V1848 Ori were carried out using the V filter result...
light curve of type EA has been found for an orbital period of 5.6 days. A further study of the syst...
We present results from analysis of combined spectroscopic and photometric data for three eclipsing ...
Analyses of 13 FEROS spectra from the ESO archive and 617 V-band photometric observations from the A...
WOS: A1993MF41200009Two-colour photoelectric observations of the eclipsing binary AT Pegasi have bee...
Context. The system V383 Sco was discovered to be an eclipsing binary star at the beginning of the t...
The main aim of this work was the first detailed analysis of an eclipsing binary system V641 Aur. Th...
The long-period eclipsing binary star V367 Cygni has been observed photoelectrically in two colours,...
HIP 7666 is a variable star newly discovered during the Hipparcos mission and classified as of unkno...
Two-colour photoelectric observations of the eclipsing binary AT Pegasi have been carried out at the...
WOS: 000325510600006The BVR photometric light curves of the eclipsing binary BD And were obtained in...
Of the billions of stars which compose a galaxy, a few will be members of the so called eclipsing bi...
Two-colour photoelectric observations of the new eclipsing binary HD 199497 are presented. Our obser...
We present ground-based photoelectric observations of the newly discovered eclipsing binary system V...
We investigate four eclipsing binary systems V508 Cyg, V719 Her, DN Aur and KN Per, selected from Be...
New observations of the eclipsing binary system V1848 Ori were carried out using the V filter result...
light curve of type EA has been found for an orbital period of 5.6 days. A further study of the syst...
We present results from analysis of combined spectroscopic and photometric data for three eclipsing ...
Analyses of 13 FEROS spectra from the ESO archive and 617 V-band photometric observations from the A...
WOS: A1993MF41200009Two-colour photoelectric observations of the eclipsing binary AT Pegasi have bee...
Context. The system V383 Sco was discovered to be an eclipsing binary star at the beginning of the t...
The main aim of this work was the first detailed analysis of an eclipsing binary system V641 Aur. Th...
The long-period eclipsing binary star V367 Cygni has been observed photoelectrically in two colours,...
HIP 7666 is a variable star newly discovered during the Hipparcos mission and classified as of unkno...
Two-colour photoelectric observations of the eclipsing binary AT Pegasi have been carried out at the...
WOS: 000325510600006The BVR photometric light curves of the eclipsing binary BD And were obtained in...