L'une des raisons du succès de la théorie de la nucléosynthèse explosive est sa capacité d'explication des rapports isotopiques terrestres et météoritiques. Une comparaison quantitative détaillée des abondances isotopiques à la source du rayonnement cosmique avec les prédictions de la nucléosynthèse serait très riche en information. Nous insisterons sur les observations et les interprétations relevantes et sur leurs limites.The great achievement of the explosive nucleosynthesis is the explanation of the isotopic abundances measured in the solar system material. A comparison between the isotopic abundances inferred at the cosmic ray source with those expected in the enveloppe of an exploded star would be interesting. We point out several key...
A model was examined in which the cosmic ray abundances of elements from C to Fe are consistent with...
The individual isotopes of galactic cosmic ray Ne, Mg, and Si at 100 MeV/nucleon were clearly resolv...
A table showing the relative abundance of chemical elements in the primary cosmic radiation, when co...
Since this is the first rapporteur talk on cosmic ray isotopes in thirteen Cosmic Ray Conferences, ...
Recent measurements of nonsolar isotopic patterns for the elements neon and (perhaps) magnesium in c...
The Cosmic Ray Isotope Spectrometer on the ACE spacecraft measures the isotopic composition of cosmi...
The Cosmic Ray Isotope Spectrometer on the ACE spacecraft measures the isotopic composition of cosmi...
New observations of galactic cosmic rays at higher energies (about 400-780 MeV nucleon^(-1)) than ob...
The study of the isotopic abundances of the rare gases helium, neon and argon in iron meteorites has...
Studies of the isotopic composition of nuclei in the cosmic radiation are reviewed, including abunda...
The study of the isotopic abundances of the rare gases helium, neon and argon in iron meteorites has...
The individual isotopes of galactic cosmic ray Ne, Mg, and Si at ~100 MeV/nucleon have been clearly...
Galactic cosmic rays represent a directly accessible sample of matter that originates outside the so...
The elemental composition of the cosmic-ray source is different from that which has been generally t...
We report new high resolution measurements of the elemental and isotopic composition of galactic co...
A model was examined in which the cosmic ray abundances of elements from C to Fe are consistent with...
The individual isotopes of galactic cosmic ray Ne, Mg, and Si at 100 MeV/nucleon were clearly resolv...
A table showing the relative abundance of chemical elements in the primary cosmic radiation, when co...
Since this is the first rapporteur talk on cosmic ray isotopes in thirteen Cosmic Ray Conferences, ...
Recent measurements of nonsolar isotopic patterns for the elements neon and (perhaps) magnesium in c...
The Cosmic Ray Isotope Spectrometer on the ACE spacecraft measures the isotopic composition of cosmi...
The Cosmic Ray Isotope Spectrometer on the ACE spacecraft measures the isotopic composition of cosmi...
New observations of galactic cosmic rays at higher energies (about 400-780 MeV nucleon^(-1)) than ob...
The study of the isotopic abundances of the rare gases helium, neon and argon in iron meteorites has...
Studies of the isotopic composition of nuclei in the cosmic radiation are reviewed, including abunda...
The study of the isotopic abundances of the rare gases helium, neon and argon in iron meteorites has...
The individual isotopes of galactic cosmic ray Ne, Mg, and Si at ~100 MeV/nucleon have been clearly...
Galactic cosmic rays represent a directly accessible sample of matter that originates outside the so...
The elemental composition of the cosmic-ray source is different from that which has been generally t...
We report new high resolution measurements of the elemental and isotopic composition of galactic co...
A model was examined in which the cosmic ray abundances of elements from C to Fe are consistent with...
The individual isotopes of galactic cosmic ray Ne, Mg, and Si at 100 MeV/nucleon were clearly resolv...
A table showing the relative abundance of chemical elements in the primary cosmic radiation, when co...