CCD Observations of the Algol-type Binary AO Serpentis

Details CCD Observations of the Algol-type Binary AO Serpentis CCD Observations of the Algol-type Binary AO Serpentis

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..848..447z&link_type=abstract

RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society. AIP Conferenc

Astronomy and Astrophysics

Astrophysics

Eclipsing Binaries, Charge-Coupled Devices, Image Detectors, And Ir Detector Arrays, Pulsations, Oscillations, And Stellar Seismology

Scientific paper

Our recent CCD observations of the short-period eclipsing binary AO Ser
are presented. The observations were performed with the 40cm Cassegrain
reflector at the Athens University Observatory, during June 2005, and
confirm that the primary component of AO Ser is a pulsating star.
Moreover,

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