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Astron. Astrophys. 327, 1039-1053 (1997)

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Acknowledgements

We are deeply endebted to our collaborators F. Allard and P. Hauschildt, for providing various model atmospheres and for numerous discussions. We are also grateful to D. Saumon and D. Alexander for providing their zero-metallicity atmosphere models and their grainless opacities, respectively, and to W. Däppen for computing zero-metallicity MHD EOS upon request. We also acknowledge useful conversations with A. Burrows in particular and with the Tucson group in general. The computation were done on the CRAY C90 of the Centre d'Etudes Nucléaire de Grenoble.

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© European Southern Observatory (ESO) 1997

Online publication: April 6, 1998
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