Results 141 to 150 of about 2,016,206 (398)
A Gravitational-wave-detectable Candidate Type Ia Supernova Progenitor
Type Ia supernovae (SNe Ia), critical for studying cosmic expansion, arise from thermonuclear explosions of white dwarfs, but their precise progenitor pathways remain unclear.
Emma T. Chickles +39 more
doaj +1 more source
Orbital Decay in an Accreting and Eclipsing 13.7 Minute Orbital Period Binary with a Luminous Donor
We report the discovery of ZTF J0127+5258, a compact mass-transferring binary with an orbital period of 13.7 minutes. The system contains a white dwarf accretor, which likely originated as a post–common envelope carbon–oxygen (CO) white dwarf, and a warm
Kevin B. Burdge +26 more
doaj +1 more source
Accreting Double White Dwarf Binaries: Implications for LISA [PDF]
We explore the long-term evolution of mass-transferring white dwarf (WD) binaries undergoing both direct-impact and disk accretion and explore implications of such systems to gravitational-wave (GW) astronomy.
K. Kremer +3 more
semanticscholar +1 more source
ABSTRACT This study presents a comparative evaluation of phosphate adsorption on pristine ZIF‐8 and Fe3O4‐doped ZIF‐8 (Fe3O4/ZIF‐8), a hybrid adsorbent combining high surface area with magnetic separability. Structural integrity and composition were confirmed using SEM, XRD, FTIR, and XPS.
Edward Hartman Ernest +10 more
wiley +1 more source
There is a striking and unexplained dearth of brown dwarf companions in close orbits (< 3AU) around stars more massive than the Sun, in stark contrast to the frequency of stellar and planetary companions.
Alexander, R. D. +8 more
core +1 more source
The white dwarf population within 40 pc of the Sun [PDF]
The white dwarf luminosity function is an important tool to understand the properties of the Solar neighborhood, like its star formation history, and its age.
García-Berro, E., Torres, S.
core +3 more sources
A 5.3-min-period pulsing white dwarf in a binary detected from radio to X-rays
I. Pelisoli +21 more
semanticscholar +1 more source
Characterizing Accreting Double White Dwarf Binaries with the Laser Interferometer Space Antenna and Gaia [PDF]
We demonstrate a method to fully characterize mass-transferring double white dwarf (DWD) systems with a helium-rich (He) white dwarf (WD) donor based on the mass–radius (M–R) relationship for He WDs. Using a simulated Galactic population of DWDs, we show
K. Breivik +5 more
semanticscholar +1 more source
Abstract A subadult Moschognathus whaitsi from the Eastern Cape Province, South Africa, was scanned using synchrotron radiation X‐ray computed tomography (SRXCT). Its subadult state allowed the cranial bones and teeth to be identified and individually reconstructed in 3D.
Tristen Lafferty +3 more
wiley +1 more source
Low Frequency Gravitational Waves from White Dwarf MACHO Binaries [PDF]
The possibility that Galactic halo MACHOs are white dwarfs has recently attracted much attention. Using the known properties of white dwarf binaries in the Galactic disk as a model, we estimate the possible contribution of halo white dwarf binaries to ...
Ben Kulick +4 more
core +2 more sources

