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astro-ph1999

On the Evolution of Cosmological Type Ia Supernovae and the Gravitational Constant

E. Garcia-Berro, E. Gaztanaga, J. Isern +2

There are at least three ways in which a varying gravitational constant could affect the interpretation of the recent high-redhisft Type Ia supernovae results. If the local val…

astro-ph1999

Possibility of the detection of classical novae with the shield of the INTEGRAL-spectrometer SPI

P. Jean, J. Gomez-Gomar, M. Hernanz +7

The shield of the INTEGRAL spectrometer provides a large detection area with a wide field-of-view. Calculations have been performed to check whether the temporal analysis of the co…

astro-ph1998

Gamma-ray emission of classical novae and its detectability by INTEGRAL

M. Hernanz, J. Gomez-Gomar, J. Jose +2

A lot of information concerning the mechanism of nova explosions will be extracted from the possible future observations with INTEGRAL. In order to be prepared for this task, we ar…

astro-ph1998

Production of the LiBeB isotopes with time-dependent GCR fluxes

Carlos Abia, Ute Lisenfeld, Jordi Isern

It is well known that no time-independent galactic cosmic ray (GCR) flux model can account for the observed linear relationship of Be and B abundances with metallicity. In this con…

astro-ph1998

Monte Carlo simulations of the disk white dwarf population

E. Garcia-Berro, S. Torres, J. Isern +1

In order to understand the dynamical and chemical evolution of our Galaxy it is of fundamental importance to study the local neighborhood. White dwarf stars are ideal candidates to…