A grid of low metallicity line-blanketed LTE model stellar atmospheres

Details A grid of low metallicity line-blanketed LTE model stellar atmospheres A grid of low metallicity line-blanketed LTE model stellar atmospheres

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.240..513h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 240, Oct. 1, 1989, p. 513-517.

Astronomy and Astrophysics

Astronomy

20

Metallicity, Stellar Atmospheres, Stellar Models, Thermodynamic Equilibrium, Atmospheric Models, Energy Distribution, Stellar Radiation, Ubv Spectra

Scientific paper

Emergent fluxes are given for a grid of low metal abundance (Z = 0.1 Z - solar) line-blanketed ATLAS 6 model atmospheres, together with corresponding UBV data and Zanstra integrals. The grid contains 101 models covering the temperature range 10,000 to 50,000 K at steps of 2000 K and log(g) from 4.5 (cgs) to the Eddington limit at steps of 0.5, with special attention paid to securing a converged model at the lowest possible log(g) for each temperature.

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