Radiative properties of stellar envelopes: Comparison of asteroseismic results to opacity calculations and measurements for iron and nickel

Autor: J. Harris, C.J. Zeippen, S. Bastiani-Ceccotti, M. Busquet, Christophe P. Blancard, P. Cossé, T. Caillaud, Jean-Christophe Pain, D. P. Kilcrease, N. H. Magee, F. Gilleron, Joyce A. Guzik, G. Faussurier, James Colgan, B. Villette, J.E. Ducreta, D. Gilles, F. Thais, G. Loisel, Chris Fontes, M. Le Pennec, Thomas Blenski, Charles Reverdin, V. Silvert, F. Delahaye, Sylvaine Turck-Chièze

Publikováno v: High Energy Density Physics
High Energy Density Physics, Elsevier, 2013, 9 (3), pp.473-479. ⟨10.1016/j.hedp.2013.04.004⟩
High Energy Density Physics, 2013, 9 (3), pp.473-479. ⟨10.1016/j.hedp.2013.04.004⟩

The international OPAC consortium consists of astrophysicists, plasma physicists and experimentalists who examine opacity calculations used in stellar physics that appear questionable and perform new calculations and laser experiments to understand t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::73177d6c488319b09b742aa983c87b85
https://hal.archives-ouvertes.fr/hal-02524629