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Results: 1-13 |
Results: 13

Authors: Gil-Pons, P Garcia-Berro, E
Citation: P. Gil-pons et E. Garcia-berro, On the formation of oxygen-neon white dwarfs in close binary systems, ASTRON ASTR, 375(1), 2001, pp. 87-99

Authors: Salaris, M Cassisi, S Garcia-Berro, E Isern, J Torres, S
Citation: M. Salaris et al., On the white dwarf distances to galactic globular clusters, ASTRON ASTR, 371(3), 2001, pp. 921-931

Authors: Corsico, AH Benvenuto, OG Althaus, LG Isern, J Garcia-Berro, E
Citation: Ah. Corsico et al., The potential of the variable DA white dwarf G117-B15A as a tool for fundamental physics, NEW ASTRON, 6(4), 2001, pp. 197-213

Authors: Isern, J Bravo, E Garcia-Berro, E Dominguez, I Salaris, M
Citation: J. Isern et al., On the internal composition of white dwarfs, NUCL PHYS A, 688(1-2), 2001, pp. 122C-125C

Authors: Isern, J Hernanz, M Garcia-Berro, E Salaris, M
Citation: J. Isern et al., White dwarfs as tracers of galactic evolution, ASTRO SP SC, 277, 2001, pp. 273-276

Authors: Isern, J Giovannelli, F Sabau, L Bravo, E Gomez-Gomar, J Hernanz, M Garcia-Berro, E La Padula, CD Gutierrez, J Jose, J Garcia-Senz, D Bausells, J Cabestany, J Madrenas, J Angulo, M Fernandez-Valbuena, M Herrera, E Reina, M Talavera, A
Citation: J. Isern et al., SIXE: An x-ray experiment for the MINISAT platform, ASTRO SP SC, 276(1), 2001, pp. 39-48

Authors: Salaris, M Garcia-Berro, E Hernanz, M Isern, J Saumon, D
Citation: M. Salaris et al., The ages of very cool hydrogen-rich white dwarfs, ASTROPHYS J, 544(2), 2000, pp. 1036-1043

Authors: Isern, J Garcia-Berro, E Hernanz, M Chabrier, G
Citation: J. Isern et al., The energetics of crystallizing white dwarfs revisited again, ASTROPHYS J, 528(1), 2000, pp. 397-400

Authors: Garcia-Berro, E Torres, S Isern, J Burkert, A
Citation: E. Garcia-berro et al., Monte Carlo simulations of the disc white dwarf population, M NOT R AST, 302(1), 1999, pp. 173-188

Authors: Ritossa, C Garcia-Berro, E Iben, I
Citation: C. Ritossa et al., On the evolution of stars that form electron-degenerate cores processed bycarbon burning. V. Shell convection sustained by helium burning, transientneon burning, dredge-out, urca cooling, and other properties of an 11 M-circle dot population I model star, ASTROPHYS J, 515(1), 1999, pp. 381-397

Authors: Isern, J Garcia-Berro, E Hernanz, M Mochkovitch, R
Citation: J. Isern et al., The physics of white dwarfs, J PHYS-COND, 10(49), 1998, pp. 11263-11272

Authors: Torres, S Garcia-Berro, E Isern, J
Citation: S. Torres et al., Neural network identification of halo white dwarfs, ASTROPHYS J, 508(1), 1998, pp. L71-L74

Authors: Isern, J Garcia-Berro, E Hernanz, M Mochkovitch, R Torres, S
Citation: J. Isern et al., The halo white dwarf population, ASTROPHYS J, 503(1), 1998, pp. 239-246
Risultati: 1-13 |