activity
19952004
most citedThe first generation of stars: first steps towards chemical evolution of galaxies

151 citations · 413 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph2004★ 73 cited

Cosmic Star Formation, Reionization, and Constraints on Global Chemical Evolution

Frederic Daigne, Keith A. Olive, Elisabeth Vangioni-Flam +2

Motivated by the WMAP results indicating an early epoch of reionization, we consider alternative cosmic star formation models which are capable of reionizing the early intergalacti…

astro-ph1999★ 80 cited

Lithium-Beryllium-Boron : Origin and Evolution

Elisabeth Vangioni-Flam, Michel Casse, Jean Audouze

The origin and evolution of Lithium-Beryllium-Boron is a crossing point between different astrophysical fields : optical and gamma spectroscopy, non thermal nucleosynthesis, Big Ba…

astro-ph1999★ 5 cited

New high S/N observations of the Li-6/Li-7 blend in HD 84937 and two other metal-poor stars

R. Cayrel, M. Spite, F. Spite +3

High S/N ratio spectra have been obtained at CFHT at a spectral resolution of 100 000 for HD 84397 and two other metal poor stars. For HD 84 937, the S/N of 650 per pixel was obtai…

astro-ph1998★ 82 cited

Lithium-6 : Evolution from Big Bang to Present

Elisabeth Vangioni-Flam, Michel Casse, Roger Cayrel +3

The primordial abundances of Deuterium, he4, and li7 are crucial to determination of the baryon density of the Universe in the framework of standard Big Bang nucleosynthesis (BBN).…

astro-ph1997★ 22 cited

Star Formation Histories versus Redshift : Consequences for Overall Metallicity and Deuterium Destruction

Michel Casse, Keith A. Olive, Elisabeth Vangioni-Flam +1

The flood of new data on deep surveys, and above all the CFRS (Canada-France-Redshift-Survey), has had a great impact on studies of galactic evolution. On the basis of cosmological…

astro-ph1995★ 151 cited

The first generation of stars: first steps towards chemical evolution of galaxies

Jean Audouze, Joseph Silk

We argue that extreme metal-poor stars show a high dispersion in metallicity, because their abundances are the outcome of very few supernova events. Abundance anomalies should appe…