Granada oscillation code (GraCo)
暂无分享,去创建一个
[1] J. Christensen-Dalsgaard,et al. Inter-comparison of the g-, f- and p-modes calculated using different oscillation codes for a given stellar model , 2007, 0711.2587.
[2] J. MacDonald,et al. The mass of helium in white dwarf stars and the formation and evolution of hydrogen-deficient post-AGB stars , 2006 .
[3] S. Allen,et al. Fe emission and ionized excess absorption in the luminous quasar 3C 109 with XMM–Newton , 2006, astro-ph/0605747.
[4] A. Moya,et al. Non-adiabatic theoretical observables in $\delta$ Scuti stars , 2003, astro-ph/0310894.
[5] A. Moya,et al. Non-adiabatic theoretical observables in δ Scuti stars , 2003 .
[6] C. Aerts,et al. Influence of non-adiabatic temperature variations on line profile variations of slowly rotating beta Cep stars and SPBs. I. Non-adiabatic eigenfunctions in the atmosphere of a pulsating star , 2002 .
[7] A. Claret. STUDIES ON STELLAR ROTATION. I. THE THEORETICAL APSIDAL MOTION FOR EVOLVEDROTATING STARS , 1999 .
[8] P. Morel. CESAM: A code for stellar evolution calculations , 1997 .
[9] R. Garrido,et al. Modal discrimination of pulsating stars by using Strömgren photometry , 1990 .
[10] H. Shibahashi,et al. Theoretical eigenfrequencies of solar oscillations of low harmonic degree l in five-minute range , 1983 .
[11] V. Zharkov,et al. The free oscillations of Jupiter and Saturn , 1976 .
[12] P. Ledoux,et al. The Nonradial Oscillations of Gaseous Stars and the Problem of Beta Canis Majoris. , 1951 .