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- Centre National de la Recherche ScientifiqueFR95 papers
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6 papers · 2 filters
Water in IRC+10216: a genuine formation process by shock-induced chemistry in the inner wind
Isabelle Cherchneff
Context: The presence of water in the wind of the extreme carbon star IRC+10216 has been confirmed by the Herschel telescope. The regions where the high-J H2O lines have been detec…
Origin of the p-Nuclei in Explosive Nucleosynthesis
T. Rauscher
A number of naturally occurring, proton-rich nuclides (the p-nuclei) cannot be made in the s- and r-process. It has been found that massive stars can produce p-nuclei through photo…
Origin of the Chemical Elements
T. Rauscher, A. Patkos
This review provides the necessary background from astrophysics, nuclear, and particle physics to understand the cosmic origin of the chemical elements. It reflects the year 2009 s…
Constraints on rotational mixing from surface evolution of light elements in massive stars
Urs Frischknecht, Raphael Hirschi, Georges Meynet +5
Context. Light elements and nitrogen surface abundances together can constrain the mixing efficiencies in massive stars on the main sequence, because moderate mixing at the surface…
The chemistry of population III supernova ejecta: II - The nucleation of molecular clusters as a diagnostic for dust in the early universe
Isabelle Cherchneff, Eli dwek
We study the formation of molecular precursors to dust in the ejecta of Population III supernovae using a chemical kinetic approach. Our work focuses on zero-metallicity 20 Msun an…
The stellar correlation function from SDSS - A statistical search for wide binary stars
M. Longhitano, B. Binggeli
We study the statistical properties of the wide binary population in the Galaxy field with projected separations larger than 200 AU by constructing the stellar angular two-point co…