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A photometric monitoring of bright high-amplitude delta Scuti stars. II. Period updates for seven stars
We present new photometric data for seven high-amplitude delta Scutistars. The observations were acquired between 1996 and 2002, mostly inthe Johnson photometric system. For one star (GW UMa), our observationsare the first since the discovery of its pulsational nature from theHipparcos data. The primary goal of this project was to update ourknowledge on the period variations of the target stars. For this, wehave collected all available photometric observations from theliterature and constructed decades-long O-C diagrams of the stars. Thistraditional method is useful because of the single-periodic nature ofthe light variations. Text-book examples of slow period evolution (XXCyg, DY Her, DY Peg) and cyclic period changes due to light-time effect(LITE) in a binary system (SZ Lyn) are updated with the newobservations. For YZ Boo, we find a period decrease instead of increase.The previously suggested LITE-solution of BE Lyn (Kiss &Szatmáry \cite{Kiss95}) is not supported with the new O-Cdiagram. Instead of that, we suspect the presence of transient lightcurve shape variations mimicking small period changes.
| Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS
Radial velocities have been determined for a sample of 2930 B2-F5 stars,95% observed by the Hipparcos satellite in the north hemisphere and 80%without reliable radial velocity up to now. Observations were obtainedat the Observatoire de Haute Provence with a dispersion of 80Ä,mm(-1) with the aim of studying stellar and galactic dynamics.Radial velocities have been measured by correlation with templates ofthe same spectral class. The mean obtained precision is 3.0 km s(-1)with three observations. A new MK spectral classification is estimatedfor all stars. Based on observations made at the Haute ProvenceObservatory, France and on data from The Hipparcos Catalogue, ESA.Tables 4, 5 and 6 are only available in electronic form at the CDS viaanonymous ftp to cdsarc.u-strasbg.fr or viahttp://cdsweb.u-strasbg.fr/Abstract.htm
| Period Changes in HD 79889
Not Available
| Stromgren photometry of the high amplitude delta Scuti starHD 79889.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1990RMxAA..20...37R&db_key=AST
| The variable star HD 79889
Observations of the variable star HD 79889 were obtained in 1986 usingthe 40 cm Cassegrain reflector at the Kvistaberg Observatory. Althoughthe light curve of the variable resembles that of a classical cepheid oran RRab variable, the short period of 0.096 days suggest that it couldbe classified as a dwarf cepheid. A high amplitude of 0.34 m in V isfound, and the present data indicate that HD 79889 is a population IDelta Scu variable.
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| Takýmyýldýz: | Buyuk Ayi |
| Sað Açýklýk: | 09h19m15.33s |
| Yükselim: | +46°56'37.6" |
| Görünürdeki Parlaklýk: | 6.883 |
| Uzaklýk: | 205.339 parsek |
| özdevim Sað Açýklýk: | -29.2 |
| özdevim Yükselim: | -18.3 |
| B-T magnitude: | 6.855 |
| V-T magnitude: | 6.881 |
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