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A catalog of rotational and radial velocities for evolved stars. II. Ib supergiant stars
Rotational velocity vsin i and mean radial velocity are presented for asample of 231 Ib supergiant stars covering the spectral region F, G andK. This work is the second part of the large survey carried out with theCORAVEL spectrometer to establish the behavior of the rotation for starsevolving off the main sequence (De Medeiros & Mayor 1999). Thesedata will add constraints to the study of the rotational behavior inevolved stars, as well as solid information concerning tidalinteractions in binary systems and on the link between rotation,chemical abundance and activity in stars of intermediate masses. Basedon observations collected at the Haute-Provence Observatory,Saint-Michel, France and at the European Southern Observatory, La Silla,Chile Table 1 is only available in electronic form at the CDS viaanonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/395/97
| Carbon, nitrogen and oxygen abundances in yellow supergiants.
Carbon, nitrogen and oxygen abundances were measured in a sample of 9yellow supergiants for which accurate rotational velocities are nowavailable. We obtain [O/Fe]=~-0.2, a result consistent with other youngobjects (main sequence B stars, planetary nebulae, H II regions). Wealso find [C/Fe]=~-0.2 for 7 stars, and =~0.0 for another 2 ones, and[N/Fe]=~0.0 for 6 stars and =~+0.2 for the other 3 ones. Stars showinglow carbon and/or high nitrogen are assumed to show convective mixingeffects. The present results seem to indicate that, among the lowrotation supergiants located near the rotational discontinuity at F9Ib,a fraction of them shows no mixing, and another fraction does showmixing effects, probably depending on their evolutionary stage.
| Photometry of F-K type bright giants and supergiants. I - Intermediate band and H-Beta observations
Over 1500 observations of 560 bright giants and supergiants of types F-Kare presented and compared to the observations by Gray and Olsen (1991).The present results include intermediate-band which is slightlydifferent from the Stromgren data by Gray and Olsen due to a differentwidth for the v filter. A systematic difference in m(1) - M(1) withdecreasing temperature is noted in the two H-Beta data sets, and thecorrelations are defined.
| Photometry of F-K type bright giant and supergiants. II - Calibration on indices in terms of luminosity reddening and abundance of F-type stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1991AJ....102.1826E&db_key=AST
| The calibration of the Stromgren photometric system for A, F and early G supergiants. I - The observational data
An empirical calibration of the Stromgren uvby-beta photometric systemfor the A, F, and early G supergiants is being derived. This paperexplains the observational program and the photometric reductiontechniques used and presents a catalog of new Stromgren photometry forover 600 A, F, and G supergiants.
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| Takýmyýldýz: | Pergel |
| Sað Açýklýk: | 14h02m04.28s |
| Yükselim: | -69°02'27.2" |
| Görünürdeki Parlaklýk: | 8.343 |
| Uzaklýk: | 315.457 parsek |
| özdevim Sað Açýklýk: | -7.2 |
| özdevim Yükselim: | -17 |
| B-T magnitude: | 8.917 |
| V-T magnitude: | 8.391 |
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