-
1
Discovery of the Richest Pulsating Ultramassive White Dwarf
Published 2025-01-01Subjects: “…White dwarf stars…”
Get full text
Article -
2
A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397
Published 2025-01-01Subjects: “…White dwarf stars…”
Get full text
Article -
3
Stability and Convergence of Nuclear Detonations in White Dwarf Collisions
Published 2025-01-01Subjects: “…White dwarf stars…”
Get full text
Article -
4
Effect of Generalized Uncertainty Principle on Main-Sequence Stars and White Dwarfs
Published 2015-01-01“…Astrophysical objects such as main-sequence stars and white dwarfs are examined and discussed as an application. …”
Get full text
Article -
5
3D Convective Urca Process in a Simmering White Dwarf
Published 2025-01-01Subjects: Get full text
Article -
6
A Multiple-detection-heads Machine Learning Algorithm for Detecting White Dwarfs
Published 2025-01-01Subjects: “…White dwarf stars…”
Get full text
Article -
7
Sporadic Dips from Extended Debris Transiting the Metal-rich White Dwarf SBSS 1232+563
Published 2025-01-01Subjects: “…White dwarf stars…”
Get full text
Article -
8
A Search for Radio Millisecond Pulsar Companions around Extremely Low-mass White Dwarfs with Ellipsoidal Variability
Published 2025-01-01Subjects: “…White dwarf stars…”
Get full text
Article -
9
The Unique Helium Nova V445 Puppis Ejected ≫0.001 M⊙ in the Year 2000 and Will Not Become a Type Ia Supernova
Published 2025-01-01“…V445 Puppis (Nova Puppis 2000) is the only known example of a helium nova, where a layer of helium-rich gas accretes onto the surface of a white dwarf (WD) in a cataclysmic variable, with runaway helium burning making for the nova event. …”
Get full text
Article -
10
Hunting for Cold Exoplanets via Microlensing
Published 2023-08-01“…Microlensing has discovered the first cold super-Earth, and the first Jupiter planet orbiting a white dwarf. It also detected a number of Earth, Super-Earth, Neptune, Saturn, Jupiter, super-Jupiter orbiting main sequence stars in the mass range 0.08 – 1M$\odot $. …”
Get full text
Article -
11
A Multiwavelength Light-curve Analysis of the Classical Nova KT Eri: Optical Contribution from a Large Irradiated Accretion Disk
Published 2025-01-01“…This result is consistent with the temporal variation of wide-band V brightness that varies almost with the intermediate-band Strömgren y brightness, because the V flux is dominated by continuum radiation, the origin of which is a photospheric emission from the very bright disk. We determined the white dwarf mass to be M _WD = 1.3 ± 0.02 M _⊙ , the hydrogen-burning turnoff epoch to be ∼240 days after the outburst, the distance modulus in the V band to be ( m − M ) _V = 13.4 ± 0.2, and the distance to KT Eri to be d = 4.2 ± 0.4 kpc for the reddening of E ( B − V ) = 0.08. …”
Get full text
Article -
12
Discovery and Detailed Study of the M31 Classical Nova AT 2023tkw: Evidence for Internal Shocks
Published 2025-01-01“…Spectral modeling suggests a low-mass white dwarf (WD) accreting slowly from a companion star. …”
Get full text
Article -
13
Distinguishing Compact Objects in Extreme-Mass-Ratio Inspirals by Gravitational Waves
Published 2025-01-01“…Therefore, our findings suggest that it is possible to distinguish primordial black holes from white dwarfs, and, under certain conditions, neutron stars can also be differentiated from primordial black holes.…”
Get full text
Article