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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.
| A List of Late-Type Stars in the Galactic Antirotation Direction
Low-resolution objective-prism spectra (1360 Å mm^-1 at Hγ) of184 late-type stars in the Galactic antirotation direction have beenobtained with the Curtis Schmidt telescope at Cerro TololoInter-American Observatory. The stars have been classified into threegroups: F6-G2, G3-K0, and K1-M8. Subsequent observations on the BV andDDO systems have been obtained. The correlation between the thin-prismclasses and the DDO classes is as expected, with no significantsystematic differences of note. A comparison of Guide Star Catalogmagnitudes, corrected to V, is also made, with favorable results. Thestars in this list are expected to be useful for studying the structureand star formation history of the Milky Way.
| Nonvariability among lambda Bootis stars
With asteroseismic techniques it is possible to investigate the interiorand the evolutionary status of stars via their frequency spectrum. Bothinformation would be very much needed for lambda Bootis stars, a groupof metal-poor Population I, A-type stars, since no conclusive theoryexists explaining the observed abundance anomalies. Geneva and Stromgrenphotometry place these stars inside the classical instability strip orat least very close to it. We therefore have started an extensivephotometric survey for pulsation in lambda Bootis stars and havediscovered so far 13 new variables. In this paper we present results forstars which presumably are constant, because we are able to establishonly an upper level for possible variability. A typical noise level of 3mmag for Stromgren b was achieved in the relevant frequency domain up to100 d^{-1}. Considering the given noise level of our survey, we concludethat at least 50% of all investigated lambda Bootis stars inside theinstability strip are pulsating, making this group remarkable comparedto stars with similar spectral types. This may suggest that a low(surface) metallicity has an influence on the pulsation Based onobservations obtained at ESO-La Silla, CTIO, SAAO, McDonald Observatory,Instituto Astrofisica Andalucia Observatory.
| Nonvariability among lambda Bootis Stars II.: SAAO (1994, 1995), CTIO (1994) and IAA (1996) Data
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| Photoelectric photometry of late type stars in the direction opposed to galactic rotation
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1974A&AS...16..269G&db_key=AST
| Régions H II de l'hémisphère austral
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1970A&AS....3....1G&db_key=AST
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Datos observacionales y astrométricos
| Constelación: | Vela |
| Ascensión Recta: | 09h13m31.18s |
| Declinación: | -49°05'40.3" |
| Magnitud Aparente: | 6.611 |
| Distancia: | 245.7 parsecs |
| Movimiento Propio en Ascensión Recta: | 29 |
| Movimiento Propio en Declinación: | -35 |
| B-T magnitude: | 8.641 |
| V-T magnitude: | 6.779 |
Catálogos y designaciones:
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