[HTML][HTML] Binary stars in the new millennium

X Chen, Z Liu, Z Han - Progress in Particle and Nuclear Physics, 2024 - Elsevier
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 …

Compact object mergers: exploring uncertainties from stellar and binary evolution with sevn

G Iorio, M Mapelli, G Costa, M Spera… - Monthly Notices of …, 2023 - academic.oup.com
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 …

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' …

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 …

Adiabatic Mass Loss in Binary Stars. V. Effects of Metallicity and Nonconservative Mass Transfer—Application in High Mass X-Ray Binaries

H Ge, CA Tout, X Chen, S Wang, J Xiong… - The Astrophysical …, 2024 - iopscience.iop.org
Binary stars are responsible for many unusual astrophysical phenomena, including some
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) …

The Common Envelope Evolution Outcome. II. Short-orbital-period Hot Subdwarf B Binaries Reveal a Clear Picture

H Ge, CA Tout, RF Webbink, X Chen… - The Astrophysical …, 2024 - iopscience.iop.org
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 …

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 …

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 …

D Belloni, M Zorotovic, MR Schreiber… - Astronomy & …, 2024 - aanda.org
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 …

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 …