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Comparative morphology of ALIVARS and RCB type stars
Some conclusions were drawn from the analysis of the following specificfeatures of the rapid Algol-Like Irregular VARiable Stars (ALIVARS): 1)general mode of variability for ALIVARS and R CrB, 2) long periods ofnearly constant brightness, 3) specific "color - V-magnitude"dependence,4) Anticorrelation between V brightness and degree ofpolarization, 5) identity of the optical properties of the RCB andALIVARS circumstellar dust, 6) cyclic light variations at normalbrighness, 7) connection between cyclic light variations and the onsetof drastic light fadings. We found that ALIVARS have some morphologicalfeatures more in common with evolved RCB-type stars rather than withyoung Herbig Ae/Be stars. Moreover, the results of the analysis of theALIVARS evolution characteristic - a) space distribution of individualALIVARS and star formation regions, b) loci on the H-R diagram, c)equivalent widths of hydrogen absorption lines, d) relative hydrogendeficiency of two ALIVARS investigated (70% of the solar abundance for V351 Ori and 30% for RZ Psc), e) mean group parameter Vsini of ALIVARS,f) luminosity of ALIVARS �alpha emission envelopes- unambiguously point that ALIVARS are not so young as Herbig Ae/Bestars and they have left the main sequence. Thus, we have encounteredthe fact of stellar mimicry: ALIVARS tend to look out as young stars,having at that time features of rather evolved stars. Relying on suchfindings, we conclude the same ALIVARS should not be further regarded asyoung stars of the HAEBES group.
| Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS
Radial velocities have been determined for a sample of 2930 B2-F5 stars,95% observed by the Hipparcos satellite in the north hemisphere and 80%without reliable radial velocity up to now. Observations were obtainedat the Observatoire de Haute Provence with a dispersion of 80Ä,mm(-1) with the aim of studying stellar and galactic dynamics.Radial velocities have been measured by correlation with templates ofthe same spectral class. The mean obtained precision is 3.0 km s(-1)with three observations. A new MK spectral classification is estimatedfor all stars. Based on observations made at the Haute ProvenceObservatory, France and on data from The Hipparcos Catalogue, ESA.Tables 4, 5 and 6 are only available in electronic form at the CDS viaanonymous ftp to cdsarc.u-strasbg.fr or viahttp://cdsweb.u-strasbg.fr/Abstract.htm
| Determination of lg G of several variable Herbig Ae/Be stars.
Echelle spectrogrammes of 19 variable Herbig Ae/Be stars were obtainedin 1988-1992 in the wavelength interval 4000-7000Å with thespectral complex ``Zebra" at the 6-m telescope of Special AstrophysicalObservatory, Russian Academy of Sciences (SAO RAS). Kurucz's models wereemployed for the analysis of the hydrogen absorption line profiles. Forall programme and standard stars lg(g) gravity parameters were obtained.The location of the stars on the "lg(g)-T_eff_" diagram does not agreewith the hypothesis that the studied objects are pre-main sequencestars.
| Morphology of a group of variable stars of the type Is(A). III - Analysis of hydrogen line profiles from high-resolution spectra
The hydrogen line profiles of nine variable stars and 2 reference starswere investigated using echelle spectra obtained with a 6-m telescope.The lg g values are determined using the Kurucz model atmospheres. It isshown that the stars investigated fall outside the main sequence on the(lg Teff, lg g) diagram.
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| Сазвежђа: | Андромеда |
| Ректацензија: | 00h05m13.00s |
| Deклинација: | +35°34'15.7" |
| Apparent магнитуда: | 6.871 |
| Даљина: | 96.618 parsecs |
| Proper motion RA: | 2 |
| Proper motion Dec: | -36.5 |
| B-T magnitude: | 7.078 |
| V-T magnitude: | 6.889 |
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