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The new space telescope Kepler and its asteroseismological targets .
We present primary and secondary asteroseismological targets for Kepler,the new NASA space mission. We derive log T_eff and logL/Lȯ values for the selected stars and we put the starsin the log L/Lȯ - log T_eff diagram. Then, we presentour program of ground-based spectroscopic and photometric observationsof the selected targets and we show first results obtained from theseobservations.
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Observation and Astrometry data
| Constellation: | Cygnus |
| Right ascension: | 19h14m44.98s |
| Declination: | +51°08'42.3" |
| Apparent magnitude: | 9.272 |
| Proper motion RA: | -20.7 |
| Proper motion Dec: | -2.8 |
| B-T magnitude: | 9.993 |
| V-T magnitude: | 9.332 |
Catalogs and designations:
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INHABITED SKY
