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HD 10054


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Detection of a classical δ Scuti star in the new eclipsing binary system HIP 7666
HIP 7666 is a variable star newly discovered during the Hipparcosmission and classified as of unknown type (ESA 1997, The Hipparcos andTycho Catalogues, ESA SP-1200). During 23 nights between July 2000 andNovember 2000, over 2300 CCD observations in the V band were obtained.These data show that the new variable is a detached eclipsing binarysystem with an orbital period of 2.37229 days. In addition, one of thecomponents undergoes very short-period oscillations with a mainpulsation frequency of 24.46 or 25.47 c/d. HIP 7666 is therefore a newmember of the rare group of detached eclipsing binary systems with aδ Scuti type component.

Four-color and H-beta photometry for O-A0 type stars in three regions near the galactic equator
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1982A&AS...49..561W&db_key=AST

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Observation and Astrometry data

Constellation:Perseus
Right ascension:01h39m30.64s
Declination:+52°16'00.3"
Apparent magnitude:8.023
Distance:292.398 parsecs
Proper motion RA:-15.9
Proper motion Dec:-20.7
B-T magnitude:8.227
V-T magnitude:8.04

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 10054
TYCHO-2 2000TYC 3290-952-1
USNO-A2.0USNO-A2 1350-01567684
HIPHIP 7729

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