activity
20052009
most citedMight Carbon-Atmosphere White Dwarfs Harbour a New Type of Pulsating Star?

30 citations · 84 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.SR20095 cited

Pulsation in carbon-atmosphere white dwarfs: A new chapter in white dwarf asteroseismology

G. Fontaine, P. Brassard, P. Dufour +2

We present some of the results of a survey aimed at exploring the asteroseismological potential of the newly-discovered carbon-atmosphere white dwarfs. We show that, in certains re…

astro-ph200830 cited

Might Carbon-Atmosphere White Dwarfs Harbour a New Type of Pulsating Star?

G. Fontaine, P. Brassard, P. Dufour

In the light of the recent and unexpected discovery of a brand new type of white dwarfs, those with carbon-dominated atmospheres, we examine the asteroseismological potential of su…

astro-ph200727 cited

Observations and asteroseismic analysis of the rapidly pulsating hot B subdwarf PG 0911+456

S. K. Randall, E. M. Green, V. Van Grootel +11

The principal aim of this project is to determine the structural parameters of the rapidly pulsating subdwarf B star PG 0911+456 from asteroseismology. Our work forms part of an on…

astro-ph200722 cited

Evidence for a merger of binary white dwarfs: the case of GD 362

E. Garcia-Berro, P. Loren-Aguilar, A. G. Pedemonte +4

GD 362 is a massive white dwarf with a spectrum suggesting a H-rich atmosphere which also shows very high abundances of Ca, Mg, Fe and other metals. However, for pure H-atmospheres…

astro-ph2006

The Boundaries of the GW Vir Stars in the Effective Temperature - Surface Gravity Domain

P. -O. Quirion, G. Fontaine, P. Brassard

We derive the theoretical red edge of the pulsating GW Vir stars by using full evolutionary calculations that involve mass loss and diffusion. We put the emphasis on the fact that…

astro-ph2005

The Potential of Multi-Colour Photometry for Pulsating Subdwarf B Stars

S. K. Randall, G. Fontaine, P. Brassard +1

We investigate the potential of multi-colour photometry for partial mode identification in both long- and short-period variable subdwarf B stars. The technique presented is based o…