activity
19972023
most citedUnderstanding the Cool DA White Dwarf, G29-38

119 citations · 695 across the 23 of their papers we have counts for

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10 papers · 1 filter

astro-ph2008

CoRoT measures solar-like oscillations and granulation in stars hotter than the Sun

E. Michel, A. Baglin, M. Auvergne +2

Oscillations of the Sun have been used to understand its interior structure. The extension of similar studies to more distant stars has raised many difficulties despite the strong…

astro-ph2008★ 64 cited

The exoplanet-host star iota Horologii: an evaporated member of the primordial Hyades cluster

S. Vauclair, M. Laymand, F. Bouchy +4

We show that the exoplanet-host star iota Horologii, alias HD17051, which belongs to the so-called Hyades stream, was formed within the primordial Hyades stellar cluster and has ev…

astro-ph2008★ 29 cited

Whole Earth Telescope observations of the hot helium atmosphere pulsating white dwarf EC 20058-5234

WET Collaboration, D. J. Sullivan, T. S. Metcalfe +22

We present the analysis of a total of 177h of high-quality optical time-series photometry of the helium atmosphere pulsating white dwarf (DBV) EC 20058-5234. The bulk of the observ…

astro-ph2007★ 53 cited

The pulsation modes of the pre-white dwarf PG 1159-035

J. E. S. Costa, S. O. Kepler, D. E. Winget +74

PG 1159-035, a pre-white dwarf with T_eff=140,000 K, is the prototype of both two classes: the PG1159 spectroscopic class and the DOV pulsating class. Previous studies of PG 1159-0…

astro-ph2007★ 39 cited

Asteroseismological constraints on the coolest GW Vir variable star (PG 1159-type)PG 0122+200

A. H. Córsico, M. M. Miller Bertolami, L. G. Althaus +2

We present an asteroseismological study on PG 0122+200, the coolest known pulsating PG1159 (GW Vir) star. Our results are based on an augmented set of the full PG1159 evolutionary…

astro-ph2007★ 5 cited

Abell 43: Longest period Planetary Nebula Nucleus variable

J. -E. Solheim, G. Vauclair, A. S. Mukadam +2

Based on 24h high speed photometry of the hybrid PG 1159 star Abell 43, we have detected 6 sighificant pulsations with periods between 2380 s and 6075 s. A short (4h) run on the al…