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Pulkovo compilation of radial velocities for 35495 stars in a common system.
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| New results of magnetic field diagnosis in HgMn stars and normal late B-type stars
We suggested in a previous paper that three HgMn stars, HD 175640, HD178065, and HD 186122, may be suspected to possess a magnetic field thatcould be larger than 2 kG. We report here new observations of thesethree stars, three more HgMn stars, and four normal late B-type stars.The search was carried out by measuring the equivalent width of the FeII lambda 6147.7 Å line relative to the equivalent width of the FeII lambda 6149.2 Å line. The observed relative differences betweenthe equivalent widths of these Fe II lines are compared with thosederived from synthetic spectra computed by neglecting magnetic fieldeffects. To investigate the effect of oscillator strength uncertaintieson the results, we computed equivalent widths by using both Fe II loggf-values taken from Kurucz & Bell (\cite{KB95}) and Fe II loggf-values taken from Raassen & Uylings (2000). The comparison of thecomputed and observed equivalent widths based on the Kurucz & Bell(\cite{KB95}) atomic data leads us to conclude that all the stars of oursample, except HD 175640, are very likely to possess a magnetic field.On the other hand, the comparison of the computed and observedequivalent widths based on the Raassen & Uylings (2000) loggf-values suggests the possible presence of magnetic fields only inthree stars, the HgMn star HD 16717 and the two normal B-type stars HD179761 and HD 186568. The latter two are those in the sample with thelargest vsin i (15 km s-1 and 18 km s-1,respectively), so that the results for them are the most uncertain ones.
| Vitesses radiales. Catalogue WEB: Wilson Evans Batten. Subtittle: Radial velocities: The Wilson-Evans-Batten catalogue.
We give a common version of the two catalogues of Mean Radial Velocitiesby Wilson (1963) and Evans (1978) to which we have added the catalogueof spectroscopic binary systems (Batten et al. 1989). For each star,when possible, we give: 1) an acronym to enter SIMBAD (Set ofIdentifications Measurements and Bibliography for Astronomical Data) ofthe CDS (Centre de Donnees Astronomiques de Strasbourg). 2) the numberHIC of the HIPPARCOS catalogue (Turon 1992). 3) the CCDM number(Catalogue des Composantes des etoiles Doubles et Multiples) byDommanget & Nys (1994). For the cluster stars, a precise study hasbeen done, on the identificator numbers. Numerous remarks point out theproblems we have had to deal with.
| Evolved GK stars near the sun. I - The old disk population
A sample of nearly two thousand GK giants with intermediate band, (R,I),DDO and Geneva photometry has been assembled. Astrometric data is alsoavailable for most of the stars. The some 800 members of the old diskpopulation in the sample yield accurate luminosities (from two sources),reddening values and chemical abundances from calibrations of thephotometric parameters. Less than one percent of the objects arepeculiar in the sense that the flux distribution is abnormal. Thepeculiarity is signaled by strong CH (and Ba II) and weak CH. The CH+stars are all spectroscopic binaries, probably with white dwarfcompanions, whereas the CH- stars are not. A broad absorption band,centered near 3500 A, is found in the CH+ stars whereas the CH- objectshave a broad emission feature in the same region. The intensity of theseabsorptions and emissions are independent of the intensity of abnormalspectral features. Ten percent of the old disk sample have a heavyelement abundance from one and a half to three times the solar value.The distribution of the heavy element abundances is nearly a normal onewith a peak near solar abundance and ranges three times to one sixthsolar. The distribution of the (U, V) velocities is independent of theheavy element abundance and does not appear to be random. Ten percent ofthe old disk stars show a CN anomaly, equally divided between CN strongand CN weak. Several stars of individual astrometric or astrophysicalimportance are isolated.
| Large and kinematically unbiased samples of G- and K-type stars. VI - Evolved stars in the Moore-Paddock-Wayman sample
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1990PASP..102..507E&db_key=AST
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| Takýmyýldýz: | Irmak |
| Sað Açýklýk: | 02h39m26.47s |
| Yükselim: | -40°44'00.1" |
| Görünürdeki Parlaklýk: | 8.719 |
| Uzaklýk: | 383.142 parsek |
| özdevim Sað Açýklýk: | 46.8 |
| özdevim Yükselim: | 6.8 |
| B-T magnitude: | 9.929 |
| V-T magnitude: | 8.819 |
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