activity
20032008
most citedMapping the ZZ Ceti Instability Strip: Discovery of 6 New Pulsators

64 citations · 125 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph200831 cited

SDSS J142625.71+575218.3: The First Pulsating White Dwarf with a Large Detectable Magnetic Field

P. Dufour, G. Fontaine, J. Liebert +2

We report the discovery of a strong magnetic field in the unique pulsating carbon-atmosphere white dwarf SDSS J142625.71+575218.3. From spectra gathered at the MMT and Keck telesco…

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-ph200664 cited

Mapping the ZZ Ceti Instability Strip: Discovery of 6 New Pulsators

A. Gianninas, P. Bergeron, G. Fontaine

As part of an ongoing program to map better the empirical instability strip of pulsating ZZ Ceti white dwarfs, we present a brief progress report based on our last observing season…

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…

astro-ph2005

Towards an Empirical Determination of the ZZ Ceti Instability Strip

A. Gianninas, P. Bergeron, G. Fontaine

We present atmospheric parameters for a large sample of DA white dwarfs that are known to be photometrically constant. For each star, we determine the effective temperature and sur…

astro-ph2005

Detailed Spectroscopic and Photometric Analysis of DQ White Dwarfs

P. Dufour, P. Bergeron, G. Fontaine

We present an analysis of spectroscopic and photometric data for cool DQ white dwarfs based on improved model atmosphere calculations. In particular, we revise the atmospheric para…