Studies in stellar evolution. I - The calculation programme and the standard solar model

Details Studies in stellar evolution. I - The calculation programme and the standard solar model Studies in stellar evolution. I - The calculation programme and the standard solar model

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....84..135h&link_type=abstract

Astronomy and Astrophysics, vol. 84, no. 1-2, Apr. 1980, p. 135-141. Research supported by the Statens Naturvidenskabelige Fors

Astronomy and Astrophysics

Astrophysics

23

Computerized Simulation, Stellar Evolution, Stellar Models, Sun, Chemical Evolution, Convective Heat Transfer, Solar Neutrinos, Stellar Mass

Scientific paper

The paper describes the results of stellar calculations performed during 1974-1978 in order to improve and extend the earlier age and mass calibrations. The physics of the stellar models is discussed, along with the consideration of the model construction procedure and computer program details. The standard solar model corresponding to the present model physics is obtained by fitting to the sun; the model requires a mixing length of 2.0 pressure scale heights and predicts a solar neutrino flux of 5.6 SNU.

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