Pulsation and binarity: SNO and uvbyβ photometry

Details Pulsation and binarity: SNO and uvbyβ photometry Pulsation and binarity: SNO and uvbyβ photometry

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..333..165r&link_type=abstract

Tidal Evolution and Oscillations in Binary Stars: Third Granada Workshop on Stellar Structure, ASP Conference Series, Vol. 333,

Astronomy and Astrophysics

Astronomy

3

Scientific paper

The main subjects in this review are: pulsation, binarity, Sierra Nevada Observatory (SNO), uvbyβ photometry, simultaneous photometry and coordinated observing campaigns. Altogether these aspects lead to fruitful results in the fields of pulsation, binarity and, in particular, in the investigation of eclipsing binary systems which include one pulsating star as one of their components. Some advantages of the uvbyβ photometry are revised within the framework of normal stars, eclipsing binaries and pulsating stars. Additional advantages are supplied by simultaneous photometry and collaboration through coordinated multisite campaigns.

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