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The multiple frequencies of the delta Scuti star V350 Peg
V350 Peg is a delta Scuti star discovered by Hipparcos (ESA\cite{esa97}). During 35 nights between July 1997 and December 2001 some7500 CCD V observations were acquired at the Monegrillo and Esteve Duranobservatories in Spain. The new data show that this star pulsates in aclose doublet of frequencies separated by 0.17 c/d (Delta f/f=3%) withsimilar amplitudes. More frequencies are excited but cannot beidentified with certainty. The period as listed in the HipparcosCatalogue is not confirmed. Also based on data obtained by the Hipparcosastrometry satellite.
| Mesures de vitesses radiales. VIII. Accompagnement AU sol DU programme d'observation DU satellite HIPPARCOS
We publish 1879 radial velocities of stars distributed in 105 fields of4^{\circ} \times 4^{\circ}. We continue the PPO series \cite[(Fehrenbachet al. 1987;]{Feh87} \cite[Duflot et al. 1990, 1992 and 1995),]{Du90}using the Fehrenbach objective prism method. Table 1 only available inelectronic form at CDS via to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/Abstract.html
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Observation and Astrometry data
| Constellation: | Pegasus |
| Right ascension: | 23h24m17.76s |
| Declination: | +30°45'05.3" |
| Apparent magnitude: | 8.056 |
| Distance: | 215.983 parsecs |
| Proper motion RA: | 26.9 |
| Proper motion Dec: | -8.3 |
| B-T magnitude: | 9.406 |
| V-T magnitude: | 8.168 |
Catalogs and designations:
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