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Иш: Axisymmetric general relativistic simulations of the accretion-induced collapse of white dwarfs
On the Evolution of Stars That Form Electron-degenerate Cores Processed by Carbon Burning. II. Isotope Abundances and Thermal Pulses in a 10 M[SUB]sun[/SUB] Model with an ONe Core and Applications to Long-Period Variables, Classical Novae, and Accretion-induced Collapse
Claudio Ritossa, E. Garcı́a–Berro, Jr. Iben Icko
Мақола19962 иқтибосABIThe Spin Periods and Rotational Profiles of Neutron Stars at Birth
Christian D. Ott, Adam Burrows, Todd A. Thompson +2
Мақола20062 иқтибосABIThe Spin Periods and Rotational Profiles of Neutron Stars at Birth
Ott, C D, Burrows, A, Thompson, T A +2
Мақола20052 иқтибосABI