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Model Atmospheres for Population Synthesis

Published online by Cambridge University Press:  07 August 2017

Robert L. Kurucz
Robert L. Kurucz*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street Cambridge, MA 02138 U.S.A.

Abstract

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I have used my newly calculated iron group line list together with my earlier atomic and molecular line data, 58,000,000 lines total, to compute new opacities for the temperature range 2000K to 200000K. Calculations have been completed at the San Diego Supercomputer Center for 56 temperatures, for 21 pressures, for microturbulent velocities 0, 1, 2, 4, and 8 km/s, for 3,500,000 wavelength points divided into 1221 intervals from 10 to 10000 nm, for scaled solar abundances [+1.0], [+0.5], [+0.3], [+0.2], [+0.1], [+0.0], [-0.1], [-0.2], [-0.3], [-0.5], [-1.0], [-1.5], [-2.0], [-2.5], [-3.0], [-3.5], [-4.0], [-4.5], and [-5.0]. I have rewritten my model atmosphere program to use the new line opacities, additional continuous opacities, and an approximate treatment of convective overshooting. The opacity calculation was checked by computing a new theoretical solar model that matches the observed irradiance. Thus far I have completed a grid of 7000 model atmospheres at 2 km/s for all the abundances, for the temperature range 3500K to 50000K, and for log g from 0.0 to 5.0. This grid will allow a consistent theoretical treatment of photometry from K stars to B stars. Fluxes are tabulated from .09 to 160 micrometers. Preliminary results are reported for many photometric systems. Work is underway on grids for other microturbulent velocities. Microturbulent velocity strongly affects the interpretation of Cepheid and RR Lyrae photometry. The models, fluxes, and colors are available on magnetic tape and will also be distributed on CD-ROMs.

Type
II. The Stellar Populations of Nearby Resolved Galaxies
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 225 - 232
Copyright
Copyright © Kluwer 

References

Adelman, S.J. and Gulliver, A.F.: 1990, Astrophys. J. 348, 712.Google Scholar
Anders, E. and Grevesse, N.: 1989, Geochimica et Cosmochimica Acta 53, 197.Google Scholar
Avrett, E.H., Kurucz, R.L., and Loeser, R.: 1984, Bull. Amer. Astron. Soc. 16, 450.Google Scholar
Buser, R. and Kurucz, R.L.: 1978, Astron. Astrophys. 70, 555.Google Scholar
Cowan, R.D.: 1968, J. Opt. Soc. Am. 58, 808.Google Scholar
Kurucz, R.L.: 1977, SAO Spec. Rep. No. 374, 170 pp.Google Scholar
Kurucz, R.L.: 1979a, Astrophys. J. Supp. Ser. 40, 1.Google Scholar
Kurucz, R.L.: 1979b, Dudley Observatory Report No. 14, ed. Davis Philip, A.G., p. 363.Google Scholar
Kurucz, R.L.: 1980, Bull. Amer. Astron. Soc. 11, 710.Google Scholar
Kurucz, R.L.: 1981, SAO Spec. Rep. No. 390, 319 pp.Google Scholar
Kurucz, R.L.: 1987, IAU Colloquium No. 95, The Second Conference on Faint Blue Stars , eds. Davis Philip, A.G., Hayes, D.S., and Liebert, J.W., L. Davis Press, Schenectady, 129.Google Scholar
Kurucz, R.L.: 1991, Stellar Atmospheres: Beyond Classical Models ed. by Crivellari, L., Hubeny, I., and Hummer, D.G., NATO ASI Series, Kluwer, Dordrecht, 440.Google Scholar
Kurucz, R.L., and Peytremann, E: 1975, SAO Spec. Rep. No. 362, 1219 pp.Google Scholar
Labs, D., Neckel, H., Simon, P.C., Thuillier, G.: 1987, Solar Phys. 107, 203.Google Scholar
Lester, J.B., Gray, R.O., and Kurucz, R.L.: 1986, Astrophys. J. Supp. Ser. 61, 509.CrossRefGoogle Scholar
Neckel, H. and Labs, D.: 1984, Solar Phys. 90, 205.CrossRefGoogle Scholar
Peterson, D.M.: 1979, Personal communication.Google Scholar
Relyea, L.J. and Kurucz, R.L.: 1978, Astrophys. J. Supp. Ser. 37, 45.Google Scholar
Tug, H., White, N. M., and Lockwood, G.W.: 1977, Astron. Astrophys. 61, 679.Google Scholar