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Orbits for five southern visual binaries
First orbits have been calculated for the visual binaries WDS00090-5400, 01061-4643, 05248-5219 and 08447-5443 (Alzner & Argyle\cite{Alz00}; Argyle & Alzner \cite{Arg01}). The current period forthe orbit of WDS 18068-4325 (Wierzbinski \cite{Wrz58}) is too short torepresent recent observations. The period has been lengthened to 450years (Alzner & Argyle \cite{Alz01}). For 00090-5400 the period is221 years with a moderate eccentricity; 01061-4643 is currently nearperiastron but is underobserved; 05248-5219 has passed periastron butthere have been no observations since 1993. The visual component of WDS08447-5443 (= delta Vel), which is not the same as the eclipsingcomponent recently discovered by Otero (\cite{Otr00a}), has anunexpectedly short period.
| The long-period companions of multiple stars tend to have moderate eccentricities
We examined the statistics of an angle gamma between the radius vectorof a visual companion of a multiple star and the vector of its apparentrelative motion in the system. Its distribution f(gamma ) is related tothe orbital eccentricity distribution in the investigated sample. Wefound that for the wide physical subsystems of the 174 objects from theMultiple Star Catalogue f(gamma ) is bell-shaped. The Monte-Carlosimulations have shown that our f(gamma ) corresponds to the populationof the moderate-eccentricity orbits and is not compatible with thelinear distribution f(e)=2e which follows from stellar dynamics andseems to hold for wide binaries. This points to the absence of highlyelongated orbits among the outer subsystems of multiple stars. Theconstraint of dynamical stability of triple systems is not sufficient toexplain the ``rounded-off'' outer orbits; instead, we speculate that itcan result from the angular momentum exchange in multiple systems duringtheir early evolution.
| A spectroscopic survey for lambda Bootis stars. II. The observational data
lambda Bootis stars comprise only a small number of all A-type stars andare characterized as nonmagnetic, Population i, late B to early F-typedwarfs which show significant underabundances of metals whereas thelight elements (C, N, O and S) are almost normal abundant compared tothe Sun. In the second paper on a spectroscopic survey for lambda Bootisstars, we present the spectral classifications of all program starsobserved. These stars were selected on the basis of their Strömgrenuvbybeta colors as lambda Bootis candidates. In total, 708 objects insix open clusters, the Orion OB1 association and the Galactic field wereclassified. In addition, 9 serendipity non-candidates in the vicinity ofour program stars as well as 15 Guide Star Catalogue stars were observedresulting in a total of 732 classified stars. The 15 objects from theGuide Star Catalogue are part of a program for the classification ofapparent variable stars from the Fine Guidance Sensors of the HubbleSpace Telescope. A grid of 105 MK standard as well as ``pathological''stars guarantees a precise classification. A comparison of our spectralclassification with the extensive work of Abt & Morrell(\cite{Abt95}) shows no significant differences. The derived types are0.23 +/- 0.09 (rms error per measurement) subclasses later and 0.30 +/-0.08 luminosity classes more luminous than those of Abt & Morrell(\cite{Abt95}) based on a sample of 160 objects in common. The estimatederrors of the means are +/- 0.1 subclasses. The characteristics of oursample are discussed in respect to the distribution on the sky, apparentvisual magnitudes and Strömgren uvbybeta colors. Based onobservations from the Observatoire de Haute-Provence, OsservatorioAstronomico di Padova-Asiago, Observatório do Pico dosDias-LNA/CNPq/MCT, Chews Ridge Observatory (MIRA) and University ofToronto Southern Observatory (Las Campanas).
| On the Variability of A0-A2 Luminosity Class III-V Stars
We study the Hipparcos Satellite photometry of A0-A2 luminosity classIII-V stars. Most are not particularly variable. A few stars for whichfurther study is desirable are identified.
| UBV Photometry of 500 Southern Stars [erratum: 1973MNSSA..32...48C]
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Datos observacionales y astrométricos
| Constelación: | Paleta del Pintor |
| Ascensión Recta: | 05h24m42.32s |
| Declinación: | -52°18'47.0" |
| Magnitud Aparente: | 6.736 |
| Distancia: | 148.148 parsecs |
| Movimiento Propio en Ascensión Recta: | -6.6 |
| Movimiento Propio en Declinación: | -28.6 |
| B-T magnitude: | 6.823 |
| V-T magnitude: | 6.744 |
Catálogos y designaciones:
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