[HTML][HTML] Binary stars in the new millennium
Binary stars are as common as single stars. Binary stars are of immense importance to
astrophysicists because that they allow us to determine the masses of the stars independent …
astrophysicists because that they allow us to determine the masses of the stars independent …
Compact object mergers: exploring uncertainties from stellar and binary evolution with sevn
Population-synthesis codes are an unique tool to explore the parameter space of massive
binary star evolution and binary compact object (BCO) formation. Most population-synthesis …
binary star evolution and binary compact object (BCO) formation. Most population-synthesis …
White dwarf binaries suggest a common envelope efficiency α∼ 1/3
P Scherbak, J Fuller - Monthly Notices of the Royal Astronomical …, 2023 - academic.oup.com
Common envelope (CE) evolution, which is crucial in creating short-period binaries and
associated astrophysical events, can be constrained by reverse modelling of such binaries' …
associated astrophysical events, can be constrained by reverse modelling of such binaries' …
Hot subdwarfs in close binaries observed from space-I. Orbital, atmospheric, and absolute parameters, and the nature of their companions
V Schaffenroth, I Pelisoli, BN Barlow, S Geier… - Astronomy & …, 2022 - aanda.org
Context. About a third of the hot subdwarfs of spectral type B (sdBs), which are mostly core-
helium-burning objects on the extreme horizontal branch, are found in close binaries with …
helium-burning objects on the extreme horizontal branch, are found in close binaries with …
Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer—Application in High Mass X-Ray Binaries
Binary stars are responsible for many unusual astrophysical phenomena, including some
important explosive cosmic events. The stability criteria for rapid mass transfer and common …
important explosive cosmic events. The stability criteria for rapid mass transfer and common …
The white dwarf binary pathways survey-IX. Three long period white dwarf plus subgiant binaries
SG Parsons, MS Hernandez, O Toloza… - Monthly Notices of …, 2023 - academic.oup.com
Virtually all binaries consisting of a white dwarf with a non-degenerate companion can be
classified as either close post-interaction systems (with orbital periods of a few days or less) …
classified as either close post-interaction systems (with orbital periods of a few days or less) …
The Common Envelope Evolution Outcome. II. Short-orbital-period Hot Subdwarf B Binaries Reveal a Clear Picture
Common envelope evolution (CEE) is vital for forming short-orbital-period compact binaries.
It covers many objects, such as double compact merging binaries, Type Ia supernovae …
It covers many objects, such as double compact merging binaries, Type Ia supernovae …
Hot subdwarfs in close binaries observed from space-II. Analyses of the light variations
V Schaffenroth, BN Barlow, I Pelisoli, S Geier… - Astronomy & …, 2023 - aanda.org
Context. Hot subdwarfs in close binaries with either M dwarf, brown dwarf, or white dwarf
companions show unique light variations. In hot subdwarf binaries with M dwarf or brown …
companions show unique light variations. In hot subdwarf binaries with M dwarf or brown …
Formation of long-period post-common envelope binaries-I. No extra energy is needed to explain oxygen-neon white dwarfs paired with AFGK-type main-sequence …
Context. It has been claimed for more than a decade that energies other than orbital and
thermodynamic internal are required to explain post-common envelope (CE) binaries with …
thermodynamic internal are required to explain post-common envelope (CE) binaries with …
Orbital parameters for an ELM white dwarf with a white dwarf companion: LAMOST J033847. 06+ 413424.2
H Yuan, Z Li, Z Bai, Y Dong, Y Cheng… - Monthly Notices of …, 2023 - academic.oup.com
Double white dwarf systems are of great astrophysical importance in the field of gravitational
wave and Type Ia supernova. While the binary fraction of CO core white dwarf is about a few …
wave and Type Ia supernova. While the binary fraction of CO core white dwarf is about a few …