Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Université de Montréal
McGill University
Montreal, Universite, Montreal, Canada
Département de Physique, Université de Montréal, Montréal, PQ, H3C 3J7, Canada ; LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France Washington, D.C.
Département de Physique, Université de Montréal, Montréal, PQ, H3C 3J7 Universite; Observatoire du Mont Megantic, Notre-Dame-des-Bois, Canada
Département de Physique, Université de Montréal, Montréal, QC, H3C 3J7, Canada; LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France Lyon, France
Montreal Univ; CERCA, Canada
Département de Physique, Université de Montréal, Montreal, QC H3C 3J7, Canada Universite; Observatoire Astronomique du Mont Megantic, Montreal, Canada
Montreal, Universiite, Montreal; Observatoire du Mont Megantic, Quebec, Canada
Montreal, Universite, Canada
LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France; Département de Physique, Université de Montréal, Montréal, PQ, H3C 3J7, Canada de Montreal, Montreal, Quebec, Canada
Montreal, Universite, Montreal; Observatoire du Mont Megantic, Quebec, Canada
Département de Physique, Université de Montréal, Montréal, PQ H3C 3J7, Canada Astronomique du Mont Megantic, Megantic, Quebec, Canada
Université de Montreal, Montreal, Canada
Département de Physique, Université de Montréal, Montreal, PQ, H3C 3J7, Canada; LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France
Montreal, Universite, Montreal; Observatoire Astronomique du Mont Megantic, Quebec, Canada
Montreal, Universite; Observatoire
A crucial test of the diffusion model - 53 Camelopardalis
A search for magnetic fields in cool sdB stars
About diffusivity, radiative viscosity and particle transport
Abundance anomalies in A and B stars and the accretion of nuclear-processed material from supernovae and evolved giants
Abundance Anomalies in Horizontal Branch Stars and Atomic Diffusion
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Profile ID: LFWR-SCP-P-158524