Browsing Exact and Earth Sciences by Subject "White dwarfs"
Now showing items 1-20 of 95
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2006 Whole Earth Telescope observations of GD358 : a new look at the prototype DBV
(2009) [Journal article]We report on the analysis of 436.1 hr of nearly continuous high-speed photometry on the pulsating DB white dwarf GD358 acquired with the Whole Earth Telescope (WET) during the 2006 international observing run, designated ... -
About the existence of warm H-rich pulsating white dwarfs
(2020) [Journal article]Context. The possible existence of warm (Teff ∼ 19 000 K) pulsating DA white dwarf (WD) stars, hotter than ZZ Ceti stars, was predicted in theoretical studies more than 30 yr ago. These studies reported the occurrence of ... -
Analysis of cool DO-type white dwarfs from the Sloan Digital Sky Survey data release 10
(2014) [Journal article]We report on the identification of 22 new cool DO-type white dwarfs (WDs) detected in data release 10 (DR10) of the Sloan Digital Sky Survey (SDSS). Among them, we found one more member of the so-called hot-wind DO WDs, ... -
An empirical test of the theory of crystallization in stellar interiors
(1997) [Journal article]Our theoretical calculations indicate that the massive pulsating DA white dwarf, BPM 37093, has a crystallized ion interior. Our estimates for the crystallized mass fraction depend on our assumption for the interior ... -
An observational limit to the evolutionary time scale of the 13,000 K white dwarf G117-B15A
(1990) [Journal article]Nature has provided us with a way of measuring the evolutionary time scale of some stars through aster oseismology, i.e., the study of stellar interiors through their intrinsic variations in brightness. By measuring the ... -
Asteroseismological study of massive ZZ Ceti stars with fully evolutionary models
(2013) [Journal article]We present the first asteroseismological study for 42 massive ZZ Ceti stars based on a large set of fully evolutionary carbon–oxygen core DA white dwarf models characterized by a detailed and consistent chemical inner ... -
Asteroseismology of PG 1541 + 651 and BPM 31594 with TESS
(2023) [Journal article]We present the photometric data from TESS for two known ZZ Ceti stars, PG 1541 + 651 and BPM 31594. Before TESS, both objects only had observations from short runs from ground-based facilities, with three and one period ... -
Asteroseismology of ZZ Ceti stars with full evolutionary white dwarf models : II. The impact of AGB thermal pulses on the asteroseismic inferences of ZZ Ceti stars
(2018) [Journal article]Context. The thermally pulsing phase on the asymptotic giant branch (TP-AGB) is the last nuclear burning phase experienced by most low- and intermediate-mass stars. During this phase, the outer chemical stratification above ... -
Asteroseismology of ZZ Ceti stars with fully evolutionary white dwarf models : I. the impact of the uncertainties from prior evolution on the period spectrum
(2017) [Journal article]Context. ZZ Ceti stars are pulsating white dwarfs with a carbon-oxygen core build up during the core helium burning and thermally pulsing Asymptotic Giant Branch phases. Through the interpretation of their pulsation periods ... -
Bpm 24754 : a new southern zz ceti star
(1998) [Journal article]We report the discovery of a new long{period ZZ Ceti star through the analysis of photometric time series gathered on 7 nights between 1995 and 1996. The light curve displays a periodic variation with a period of ~ 18 min ... -
A comparative analysis of the observed white dwarf cooling sequence from globular clusters
(2016) [Journal article]We report our study of features at the observed red end of the white dwarf cooling sequences for three Galactic globular clusters: NGC 6397, 47 Tucanae and M 4. We use deep colour– magnitude diagrams constructed from ... -
Comparing the asteroseismic properties of pulsating pre-extremely low mass white dwarf and δ Scuti stars
(2018) [Journal article]Context. Pulsating extremely low-mass pre-white dwarf stars (pre-ELMV), with masses between ~0.15 M⊙ and ~0.30 M⊙, constitute a new class of variable stars showing g- and possibly p-mode pulsations with periods between 320 ... -
Constraining the evolution of ZZ Ceti
(2003) [Journal article]We report our analysis of the stability of pulsation periods in the DAV star (pulsating hydrogen atmosphere white dwarf ) ZZ Ceti, also called R548. On the basis of observations that span 31 years, we conclude that the ... -
Convection and rotation boosted prescription of magnetic braking application to the formation of extremely low-mass white dwarfs
(2021) [Journal article]Extremely low-mass white dwarfs (ELM WDs) are the result of binary evolution in which a low-mass donor star is stripped by its companion leaving behind a helium-core white dwarf (WD). We explore the formation of ELM WDs ... -
DB white dwarfs in the Sloan Digital Sky Survey data release 10 and 12
(2015) [Journal article]Aims. White dwarfs with helium-dominated atmospheres (spectral types DO, DB) comprise approximately 20% of all white dwarfs. There are fewer studies than of their hydrogen-rich counterparts (DA) and thus several questions ... -
Direct measurement of a secular pulsation period change in the pulsating hot pre-white dwarf PG 1159-035
(1999) [Journal article]GW Vir (PG 1159[035) is the prototype of the class of multiperiodic, nonradially pulsating hot white dwarfs, and shows a strong pulsation mode at 516 s. All measurements to date of the secular variation of the 516 s pulsation ... -
Discovery of a new AM CVn system with the Kepler satellite
(2011) [Journal article]We report the discovery of a new AM CVn system on the basis of broadband photometry obtained with the Kepler satellite supplemented by ground-based optical spectroscopy. Initially retained on Kepler target lists as a ... -
Discovery of a new PG 1159 (GW Vir) pulsator
(2014) [Journal article]We report the discovery of pulsations in the spectroscopic PG 1159 type pre-white dwarf SDSS J075415.12 + 085232.18. Analysis of the spectrum by Werner et al. indicated Teff = 120 000 ± 10 000 K, log g = 7.0 ± 0.3, mass ... -
Discovery of an ultramassive pulsating white dwarf
(2013) [Journal article]We announce the discovery of themostmassive pulsating hydrogen-atmosphere white dwarf (WD) ever discovered, GD 518. Model atmosphere fits to the optical spectrum of this star show it is a 12,030 ± 210 K WD with a log g = ... -
Discovery of five new massive pulsating white dwarf stars
(2013) [Journal article]Using the SOuthern Astrophysical Research telescope (SOAR) Optical Imager at the SOAR 4.1 m telescope, we report on the discovery of five new massive pulsating white dwarf stars. Our results represent an increase of about ...