Pulsating white dwarfs: new insights

AH Córsico, LG Althaus, MM Miller Bertolami… - The Astronomy and …, 2019 - Springer
Stars are extremely important astronomical objects that constitute the pillars on which the
Universe is built, and as such, their study has gained increasing interest over the years …

Pulsating white dwarf stars and precision asteroseismology

DE Winget, SO Kepler - Annu. Rev. Astron. Astrophys., 2008 - annualreviews.org
Galactic history is written in the white dwarf stars. Their surface properties hint at interiors
composed of matter under extreme conditions. In the forty years since their discovery …

[HTML][HTML] Automated supervised classification of variable stars-I. methodology

J Debosscher, LM Sarro, C Aerts, J Cuypers… - Astronomy & …, 2007 - aanda.org
Context. The fast classification of new variable stars is an important step in making them
available for further research. Selection of science targets from large databases is much …

HS 2331+ 3905: The cataclysmic variable that has it all

S Araujo-Betancor, BT Gänsicke, HJ Hagen… - Astronomy & …, 2005 - aanda.org
We report detailed follow-up observations of the cataclysmic variable HS 2331+ 3905,
identified as an emission-line object in the Hamburg Quasar Survey. An orbital period of …

Pulsating hydrogen-deficient white dwarfs and pre-white dwarfs observed with TESS-I. Asteroseismology of the GW Vir stars RX J2117+ 3412, HS 2324+ 3944, NGC …

AH Córsico, M Uzundag, SO Kepler, LG Althaus… - Astronomy & …, 2021 - aanda.org
Context. The recent arrival of continuous photometric observations of unprecedented quality
from space missions has strongly promoted the study of pulsating stars and caused great …

Seismological studies of ZZ Ceti stars–I. The model grid and the application to individual stars

BG Castanheira, SO Kepler - Monthly Notices of the Royal …, 2008 - academic.oup.com
We calculate and explore an extensive adiabatic model grid for pulsating white dwarfs with
hydrogen-dominated atmospheres, the ZZ Ceti stars. We also compared the computed …

Kepler and TESS Observations of PG 1159-035

GO da Rosa, SO Kepler, AH Córsico… - The Astrophysical …, 2022 - iopscience.iop.org
PG 1159-035 is the prototype of the PG 1159 hot (pre-) white dwarf pulsators. This important
object was observed during the Kepler satellite K2 mission for 69 days in 59 s cadence …

KIC 11911480: the second ZZ Ceti in the Kepler field

S Greiss, BT Gänsicke, JJ Hermes… - Monthly Notices of …, 2014 - academic.oup.com
We report the discovery of the second pulsating hydrogen-rich (DA) white dwarf in the
Kepler field, KIC 11911480. It was selected from the Kepler-INT Survey (KIS) on the basis of …

Pulsational instabilities in accreting white dwarfs

P Arras, DM Townsley, L Bildsten - The Astrophysical Journal, 2006 - iopscience.iop.org
The detection of g-mode pulsations in accreting white dwarfs (WDs) in cataclysmic variables
(CVs) with a large range of effective temperatures (T eff) has shown these WDs to be a more …

GD358: three decades of observations for the in-depth asteroseismology of a DBV star

A Bischoff-Kim, JL Provencal, PA Bradley… - The Astrophysical …, 2019 - iopscience.iop.org
We report on the analysis of 34 years of photometric observations of the pulsating helium
atmosphere white dwarf GD358. The complete data set includes archival data from 1982 to …