activity
19962001
collaborators
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astro-ph2001

Upper limits of the Na yield from O-Ne nova

P. Jean, J. Knödlseder, P. von Ballmoos +3

The radioactive isotope Na is one of the primary tracer isotopes that may potentially be detectable by gamma-ray spectroscopy. This isotope is predicted to be produced in ON…

astro-ph2001

Prospects for detectability of classical novae with INTEGRAL

M. Hernanz, J. Gomez-Gomar, J. Jose +1

Classical novae are potential gamma-ray emitters, both in lines and in a continuum. Continuum emission (at energies between 20-30 and 511 keV) and line emission at 511 keV are rela…

astro-ph2001

Explosive nucleosynthesis

M. Hernanz

Many radioactive nuclei relevant for gamma-ray astrophysics are synthesized during explosive events, such as classical novae and supernovae. A review of recent results of explosive…

astro-ph1999

Galactic distribution of 1.275 MeV emission from O-Ne novae

P. Jean, M. Hernanz, J. Gomez-Gomar +1

Modelisations of galactic 1.275 MeV emission produced by the decay 22Na have been performed for several frequency-spatial distributions of ONe novae. Recent results of nova rates a…

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-ph1996

On the ^7 Li and ^7 Be synthesis in novae

M. Hernanz, J. Jose, A. Coc +1

The production of ^7 Li and ^7 Be during the explosive hydrogen-burning that occurs in nova explosions is computed by means of a hydrodynamic code able to treat both the accretion…