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Inaccuracies in the spectral classification of stars from the Tycho-2 Spectral Type Catalogue We compare the spectroscopic and trigonometric parallaxes of commonstars from the Tycho-2 Spectral Type and Hipparcos Catalogues. Thiscomparison has revealed that the distance estimations for theoverwhelming majority of stars by both methods yield very similarresults. However, there is a small fraction of stars for which thedistance estimates differ significantly. It is these stars that are thesubject of our study. We have been able to find the causes of thesedifferences.
 
  |  New periodic variables from the Hipparcos epoch photometry Two selection statistics are used to extract new candidate periodicvariables from the epoch photometry of the Hipparcos catalogue. Theprimary selection criterion is a signal-to-noise ratio. The dependenceof this statistic on the number of observations is calibrated usingabout 30000 randomly permuted Hipparcos data sets. A significance levelof 0.1 per cent is used to extract a first batch of candidate variables.The second criterion requires that the optimal frequency be unaffectedif the data are de-trended by low-order polynomials. We find 2675 newcandidate periodic variables, of which the majority (2082) are from theHipparcos`unsolved' variables. Potential problems with theinterpretation of the data (e.g. aliasing) are discussed.
 
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Observation and Astrometry data
| Constellation: | Schütze |  
    | Right ascension: | 19h31m25.11s |  
    | Declination: | -13°58'41.2" |  
    | Apparent magnitude: | 8.746 |  
    
        | Distance: | 182.149 parsecs |  
        
    
    | Proper motion RA: | 18.8 |  
    | Proper motion Dec: | -6.5 |  
    | B-T magnitude: | 10.559 |  
    | V-T magnitude: | 8.896 |  
    
 
 
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