1k citations
- B. Åsman8 profiles90 · h 98
- A. Sopczak2 profiles89 · h 83
- M. Begalli6 profiles89 · h 68
- M. Besançon2 profiles88 · h 132
- P. Verdier2 profiles88 · h 114
- D. Wicke6 profiles87 · h 64
- P. Jonsson9 profiles86 · h 54
- Y. Arnoud2 profiles85 · h 42
- L. Mundim2 profiles75 · h 124
- A. Meyer3 profiles68 · h 142
- D. Schaile8 profiles68 · h 87
- A. Quadt8 profiles67 · h 86
- Stockholm UniversitySE108 papers
- Centre National de la Recherche ScientifiqueFR104 papers
- Joint Institute for Nuclear ResearchRU100 papers
- University of WuppertalDE98 papers
- Charles UniversityCZ92 papers
- Iowa State UniversityUS92 papers
- Lancaster UniversityGB91 papers
- Sorbonne UniversitéFR90 papers
- Universidade do Estado do Rio de JaneiroBR90 papers
- Lyon 1 UniversitéFR88 papers
- FZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicCZ85 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR85 papers
Showing 2005 · astro-phShow all
2 papers · 2 filters
astro-ph2005★ 566 cited
Nucleosynthetic signatures of the first stars
Anna Frebel, Wako Aoki, Norbert Christlieb +16
The chemically most primitive stars provide constraints on the nature of the first stellar objects that formed in the Universe; elements other than hydrogen, helium and traces of l…
astro-ph2005★ 20 cited
A Link Between the Semi-Major Axis of Extrasolar Gas Giant Planets and Stellar Metallicity
R. Pinotti, L. Arany-Prado, W. Lyra +1
The fact that most extrasolar planets found to date are orbiting metal-rich stars lends credence to the core accretion mechanism of gas giant planet formation over its competitor,…