Chabrier, Gilles, Brassard, Pierre, Fontaine, Gilles, Saumon, Didier
We present new cooling sequences, color-magnitude diagrams, and color-color diagrams for cool white dwarfs with pure hydrogen atmospheres down to an effective temperature $\\te=1500$ K. We include a...
Chabrier, Gilles, Brassard, Pierre, Fontaine, Gilles, Saumon, Didier
We present new cooling sequences, color-magnitude diagrams, and color-color diagrams for cool white dwarfs with pure hydrogen atmospheres down to an effective temperature $\te=1500$ K. We include a...
Chabrier, Gilles, Brassard, Pierre, Fontaine, Gilles, Saumon, Didier
We present new cooling sequences, color-magnitude diagrams, and color-color diagrams for cool white dwarfs with pure hydrogen atmospheres down to an effective temperature $\\te=1500$ K. We include a...
Chabrier, Gilles, Brassard, Pierre, Fontaine, Gilles, Saumon, Didier
We present new cooling sequences, color-magnitude diagrams, and color-color diagrams for cool white dwarfs with pure hydrogen atmospheres down to an effective temperature $\\te=1500$ K. We include a...
The Potential of Asteroseismology for Hot, Subdwarf B Stars: A New Class of Pulsating Stars? (1996)
Charpinet, Stephane, Fontaine, Gilles, Brassard, Pierre, Dorman, Ben
We present key sample results of a systematic survey of the pulsation properties of models of hot B subdwarfs. We use equilibrium structures taken from detailed evolutionary sequences of solar...
Measuring the energy budget of a plant in a closed system--[microform] /--Pierre Brassard. (1981)
Thesis (M. Sc.)--Concordia University, 1980.
Measuring the energy budget of a plant in a closed system / (1979)
Thesis (M.Sc.)--Concordia University.