SIMBAD references

2005A&A...434.1063E - Astronomy and Astrophysics, volume 4341063-1068 (2005/5-2)

Detection of a classical δ Scuti star in the new eclipsing binary system HIP 7666.

ESCOLA-SIRISI E., JUAN-SAMSO J., VIDAL-SAINZ J., LAMPENS P., GARCIA-MELENDO E., GOMEZ-FORRELLAD J.M. and WILS P.

Abstract (from CDS):

HIP 7666 is a variable star newly discovered during the Hipparcos mission and classified as of unknown type (ESA, The Hipparcos and Tycho Catalogues, ESA SP-1200, 1997HIP...C......0E). During 23 nights between July 2000 and November 2000, over 2300 CCD observations in the V band were obtained. These data show that the new variable is a detached eclipsing binary system with an orbital period of 2.37229 days. In addition, one of the components undergoes very short-period oscillations with a main pulsation frequency of 24.46 or 25.47c/d. HIP 7666 is therefore a new member of the rare group of detached eclipsing binary systems with a δ Scuti type component.

Abstract Copyright: ∼

Journal keyword(s): stars: binaries: eclipsing - stars: oscillations - stars: variables: δ Sct - stars: individual: HIP 7666

Simbad objects: 6

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