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Astrophysics and Space Science

, Volume 136, Issue 2, pp 351–361 | Cite as

The curve of growth for stars in the effective temperature range 4000–8500 K

  • M. Villada
  • L. Rossi
Article

Abstract

A comparison of different curves of growth derived from available model atmospheres has been done. We found that, in the effective temperature range (4000–8500 K), the differences between models with the same (Teff, logg) from different authors, do not affect the shape of the curve of growth. Moreoyer, the shifts needed to superpose the curves, for different elements, differ only slightly when model from different authors are used. Then, in the low-temperature range and for the gravities we considered, the particular model atmosphere used to draw the curve of growth is not the main constrain of the method.

Keywords

Atmosphere Effective Temperature Model Atmosphere Effective Temperature Range 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company 1987

Authors and Affiliations

  • M. Villada
    • 1
    • 2
  • L. Rossi
    • 3
  1. 1.Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET)Buenos Aires
  2. 2.Observatorio Astronomico de la Universidad Nacional de CorbodaCordobaArgentina
  3. 3.Instituto Astrofisica SpazialeCNRFrascatiItaly

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