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Aufsuchkarten fur intrinsic Variable Stars in Brno.
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| Stars with the Largest Hipparcos Photometric Amplitudes
A list of the 2027 stars that have the largest photometric amplitudes inHipparcos Photometry shows that most variable stars are all Miras. Thepercentage of variable types change as a function of amplitude. Thiscompilation should also be of value to photometrists looking forrelatively unstudied, but large amplitude stars.
| Studies of Yellow Semiregular(SRd) Variables
We have used the Hipparcos database of epoch photometry to study thevariability of several yellow semiregular(SRd) variables. For some ofthe stars (V847 Cas, RW Cep, BM Sco, CE Vir), the results wereinconclusive. For SX Lac and TY Vir, the periods found were consistentwith the General Catalogue of Variable Stars (190 and 50 daysrespectively). For UU Her, the known periods of about 45 and 72 dayswere recovered. For WY And, RU Cep, and SX Her, reliable periods werefound; we used archival data to construct (O-C) diagrams to study boththe random and systematic period changes in these three stars.
| The kinematics of semiregular red variables in the solar neighbourhood.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972MNRAS.158...23F&db_key=AST
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Observation and Astrometry data
| Constellation: | Lacerta |
| Right ascension: | 22h55m59.98s |
| Declination: | +35°11'44.7" |
| Apparent magnitude: | 8.207 |
| Distance: | 645.161 parsecs |
| Proper motion RA: | -11.9 |
| Proper motion Dec: | 6.6 |
| B-T magnitude: | 10.19 |
| V-T magnitude: | 8.371 |
Catalogs and designations:
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