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Empirical Luminosities and Radii of Early-Type Stars after Hipparcos

Wybrane pełne teksty z tego czasopisma
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Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
Using Hipparcos parallaxes we derive empirical luminosities and radii of the early-type stars for which the effective temperatures are known from directly measured angular diameters and total absolute fluxes. The empirical luminosities allow a direct comparison of the position of these stars in the fundamental HR diagram with evolutionary tracks. The comparison shows an overall agreement with the Y=0.30 and Z=0.02 tracks computed with OPAL opacities and moderate amount of overshooting from the convective core. In addition, we present evidence that systematic errors of the masses read off the evolutionary tracks are below 10%. Consequently, the surface gravities obtained from these "evolutionary" masses and the empirical radii are very nearly model-independent. Spectrographic and photometric observations of these stars can therefore be used for verifying model atmospheres and calibrating photometric log g indices.
Czasopismo
Rocznik
Strony
369--380
Opis fizyczny
Bibliogr. 27 poz., tab., wykr.
Twórcy
  • Wrocław University Observatory, Kopernika 11, 51-622 Wrocław, Poland
  • Wrocław University Observatory, Kopernika 11, 51-622 Wrocław, Poland
Bibliografia
  • Allen, C.W. 1973, "Astrophysical Quantities", 3rd ed. London: Athlone Press, p. 169.
  • Andersen, J. 1991, Astron. Astrophys. Rev., 3, 91.
  • Beeckmans, F. 1977, Astron. Astrophys., 60, 1.
  • Breger, M., and Pamyatnykh, A.A. 1998, Astron. Astrophys., 332, 958.
  • Claret, A., and Giménez, A. 1992, Astron. Astrophys. Suppl. Ser., 96, 255.
  • Code, A.D., Davis, J., Bless, R.C., and Hanbury Brown, R. 1976, Astrophys. J., 203, 417 (CDBH).
  • Crowther, P.A. 1997, in: "Fundamental Stellar Properties", Proc. IAU Symp., 189, Eds. Bedding, T.R., Booth, A.J., and Davis, J., Kluwer, Dordrecht, p. 137.
  • ESA 1997, "The Hipparcos and Tycho Catalogues", ESA SP-1200.
  • Fliegner, J., and Langer, N. 1994, in: "Pulsation, Rotation and Mass Loss in Early-Type Stars", Proc. IAU Symp., 162, Eds. Balona, L.A., Henrichs, F.H., and Le Contel, J.M., Kluwer, Dordrecht, p. 147.
  • Gatewood, G.D., and Gatewood, C.V. 1978, Astrophys. J., 225, 191.
  • Girard, T.M., et al. 2000, Astron. J., 119, 2428.
  • Griffin, R.E.M., Griffin, R.F., Schröder, K.-P., and Reimers, D. 1990, Astron. Astrophys., 234, 284.
  • Griffin, R.E.M., Schröder, K.-P., Misch, A., and Griffin, R.F. 1992, Astron. Astrophys., 254, 289.
  • Griffin, R.E.M., Hünsch, M., Marshall, K.P., Griffin, R.F., and Schröder, K.-P. 1993, Astron. Astrophys., 274, 225.
  • Griffin, R.E.M., Marshall, K.P., Griffin, R.F., and Schröder, K.-P. 1995, Astron. Astrophys., 301, 217.
  • Hanbury Brown, R., Davis, J., and Allen, L.R. 1974, MNRAS, 167, 121.
  • Herbison-Evans, D., Hanbury Brown, R., Davis, J., and Allen, L.R. 1971, MNRAS, 151, 161.
  • Hoffleit, D. 1982, "The Bright Star Catalogue", Yale University Observatory, New Haven, Connecticut, U.S.A.
  • Irwin, A.W., et al. 1992, P.A.S.P., 104, 489.
  • Lutz, T.E., and Kelker, D.H. 1973, P.A.S.P., 85, 573.
  • Pamyatnykh, A.A., Dziembowski, W.A., Handler, G., and Pikall, H. 1998, Astron. Astrophys., 333, 141.
  • Rogers, F.J., and Iglesias, C.A. 1992, Astrophys. J. Suppl. Ser., 79, 507.
  • Schaller, G., Schaerer, D., Meynet, G., and Maeder, A. 1992, Astron. Astrophys. Suppl. Ser., 96, 269.
  • Schönberner, D., and Harmanec, P. 1995, Astron. Astrophys., 294, 509.
  • Smalley, B., and Dworetsky, M.M. 1995, Astron. Astrophys., 293, 446.
  • Smith, H. 1987, Astron. Astrophys., 188, 233.
  • Trumpler, R.J., and Weaver, H.F. 1953, "Statistical Astronomy" University of California Press, Berkeley, p. 369.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-a09eae2e-7892-4d7f-af79-832505c1cc5b
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