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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.
| Miscellaneous spectroscopic notes
Results of slit-spectrograph observations are reported for approximately260 stars. The data presented range from recognition of many new Ap, Am,and other unusual stars to H-alpha observations of early-typesupergiants and Be stars. The material discussed was obtained over thepast 40 years at a number of U.S. observatories and at the DominionAstrophysical Observatory in Victoria, B.C.
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| Takýmyýldýz: | Zurafa |
| Sað Açýklýk: | 07h54m20.48s |
| Yükselim: | +71°04'45.3" |
| Görünürdeki Parlaklýk: | 7.336 |
| Uzaklýk: | 178.253 parsek |
| özdevim Sað Açýklýk: | -34.1 |
| özdevim Yükselim: | -34.1 |
| B-T magnitude: | 7.34 |
| V-T magnitude: | 7.337 |
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