Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
University of Montreal
UdeM
Universite de Montreal
Lockheed Martin Canada
Départment de Physique, Université de Montréal, Canada;
Département de Physique, Université de Montréal, CP 6128, Succ. Centre-Ville, Montréal, QC, H3C 3J7, Canada Universite, Montreal, Canada; Steward Observatory, Tucson, AZ
Universite de Montreal, Montreal, Quebec, Canada
Département de Physique, Université de Montréal, C.P. 6128, Succ. Centre-Ville, Montréal, Québec, Canada H3C 3J7 de Physique, Université de Montréal, C.P. 6128, Succ. Centre-Ville, Montréal, QC H3C 3J7, Canada of Arizona, Tucson, AZ
Montreal, Universite; Observatoire du Mont Megantic, Montreal, Canada
Universite de Montreal, Montreal, Quebeca, Canada
Montreal Univ., Canada
U. Montréal
Département de Physique, Université de Montréal, P.O. Box 6128, Station Centreville, Montréal, QC H3C 3J7, Canada.
Département de Physique, Université de Montréal, Montréal, Québec H3C 3J7, Canada
Département de Physique, Université de Montréal, Québec, Canada
Département de Physique, Université de Montréal, C. P. 6128, Succ. Centre-Ville, Montréal, Québec H3C 3J7, Canada
Département de Physique, Université de Montréal, C.P. 6128, Succursale Centre-Ville, Montréal, QC H3C 3J7, Canada
Université de Montréal, Succursale Centre-Ville, Montreal, Canada
Montreal, Universiite, Montreal; Observatoire du Mont Megantic, Quebec, Canada
Steward Observatory, Tucson, AZ; Montreal, Universite, Montreal, Canada
Département de Physique, Université de Montréal, Succ. Centre-Ville, C.P. 6128, Montréal, QC H3C 3J7, Canada
Département de Physique, Université de Montréal, C.P. 6128, Succ. Centre-Ville, Montréal, QC H3C 3J7, Canada; Lockheed Martin Canada, 6111 Avenue Royalmount, Montréal, QC H4P 1K6, Canada
A Census of White Dwarfs Within 40 Parsecs of the Sun
A Comparative Study of Optical and Ultraviolet Effective Temperatures for DA White Dwarfs from the IUE Archive
A Comparison of Atmospheric Parameters for Subdwarf B Stars Derived from Lyman and Balmer-Line Analyses
A complete census of Galactic white dwarfs to 40 parsecs of the Sun.
A Comprehensive Spectroscopic Analysis of DB White Dwarfs
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