Models of Procyon A including seismic constraints
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چکیده
منابع مشابه
ar X iv : a st ro - p h / 05 01 27 0 v 1 1 4 Ja n 20 05 Models of Procyon A including seismic constraints
Detailed models of Procyon A based on new asteroseismic measurements by Eggen-berger et al. (2004b) have been computed using the Geneva evolution code including shellular rotation and atomic diffusion. By combining all non–asteroseismic observ-ables now available for Procyon A with these seismological data, we find that the observed mean large spacing of 55.5 ± 0.5 µHz favours a mass of 1.497 M...
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T. Nicholson,1 Ó. Gudmundsson2 and M. Sambridge3 1Research School of Earth Sciences, Australian National University, Canberra ACT 0200, Australia. E-mail: [email protected] 2Danish Lithospheric Centre, Øster Voldgade 20, 1350 Copenhagen K, Denmark. E-mail: [email protected] 3Centre for Advanced Data Inference, Research School of Earth Sciences, Australian National University, Canberra ACT 0200, A...
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ژورنال
عنوان ژورنال: New Astronomy
سال: 2005
ISSN: 1384-1076
DOI: 10.1016/j.newast.2004.10.002