Results 71 to 80 of about 2,016,206 (398)

Electromagnetic Characterization of the LISA Verification Binary ZTF J0526+5934

open access: yesThe Astrophysical Journal, 2023
We present an analysis of new and archival data to the 20.506 minute LISA verification binary J052610.42+593445.32 (J0526+5934). Our joint spectroscopic and photometric analysis finds that the binary contains an unseen M _1 = 0.89 ± 0.11 M _⊙ CO-core ...
Alekzander Kosakowski   +3 more
doaj   +1 more source

Cooling Process of White Dwarf Stars in Palatini f(R) Gravity

open access: yesUniverse, 2022
A simple cooling model of white dwarf stars is re-analyzed in Palatini f(R) gravity. Modified gravity affects the white dwarf structures and consequently their ages.
Surajit Kalita   +2 more
doaj   +1 more source

Can the rapid braking of the white dwarf in AE Aquarii be explained in terms of the gravitational wave emitter mechanism? [PDF]

open access: yes, 2002
The spin-down power of the white dwarf in the close binary AE Aquarii significantly exceeds the bolometric luminosity of the system. The interpretation of this phenomenon in terms of the gravitational-wave emitter mechanism has been recently suggested by
Beskrovnaya, Nina G., Ikhsanov, Nazar R.
core   +2 more sources

A White Dwarf with Transiting Circumstellar Material Far outside the Roche Limit

open access: yesAstrophysical Journal, 2019
We report the discovery of a white dwarf exhibiting deep, irregularly shaped transits, indicative of circumstellar planetary debris. Using Zwicky Transient Facility DR2 photometry of ZTF J013906.17+524536.89 and follow-up observations from the Las ...
Z. Vanderbosch   +11 more
semanticscholar   +1 more source

A radio-pulsing white dwarf binary star [PDF]

open access: yesNature, 2016
White dwarfs are compact stars, similar in size to Earth but approximately 200,000 times more massive. Isolated white dwarfs emit most of their power from ultraviolet to near-infrared wavelengths, but when in close orbits with less dense stars, white ...
T. Marsh   +28 more
semanticscholar   +1 more source

Cubic crystal elastic constants of a white dwarf stellar core determined via modal analysis

open access: yesAIP Advances, 2021
In this work, we present the cubic crystal elastic constants of a fully crystallized white dwarf stellar core. Elastic constants were calculated utilizing modal analysis of three-dimensional single-layer and stratified multi-layer crystalline core models.
K. A. Pestka II   +3 more
doaj   +1 more source

Hot white dwarfs and the UV delay in dwarf novae

open access: yes, 1998
We calculate the effect of illumination of dwarf nova accretion discs by radiation from a hot, central, white dwarf. We show that only for very hot white dwarfs (Teff ~ 40 000$ K) the inner region of quiescent dwarf nova discs are partially depleted so ...
Dubus, G.   +2 more
core   +2 more sources

A Dark Spot on a Massive White Dwarf [PDF]

open access: yes, 2015
We present the serendipitous discovery of eclipse-like events around the massive white dwarf SDSS J152934.98+292801.9 (hereafter J1529+2928). We selected J1529+2928 for time-series photometry based on its spectroscopic temperature and surface gravity ...
Bell, Keaton J.   +9 more
core   +2 more sources

Prospects for detection of detached double white dwarf binaries with Gaia, LSST and LISA [PDF]

open access: yes, 2017
Double white dwarf (DWD) binaries are expected to be very common in the Milky Way, but their intrinsic faintness challenges the detection of these systems. Currently, only a few tens of detached DWDs are know.
V. Korol   +5 more
semanticscholar   +1 more source

A Photometric and Spectroscopic Investigation of the DB White Dwarf Population Using SDSS and Gaia Data [PDF]

open access: yesAstrophysical Journal, 2019
We present a comprehensive analysis of DB white dwarfs drawn from the Sloan Digital Sky Survey, based on model fits to ugriz photometry and medium-resolution spectroscopy from the Sloan Digital Sky Survey.
C. Genest-Beaulieu, P. Bergeron
semanticscholar   +1 more source

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