The Evolution of Massive Binary Stars

P Marchant, J Bodensteiner - Annual Review of Astronomy and …, 2023 - annualreviews.org
Massive stars play a major role in the evolution of their host galaxies and serve as important
probes of the distant Universe. It has been established that the majority of massive stars …

[HTML][HTML] Fifty Years After the Discovery of the First Stellar-Mass Black Hole: A Review of Cyg X-1

J Jiang - Galaxies, 2024 - mdpi.com
Around 50 years ago, the famous bet between Stephen Hawking and Kip Thorne on
whether Cyg X-1 hosts a stellar-mass black hole became a well-known story in the history of …

Population synthesis of Be X-ray binaries: metallicity dependence of total X-ray outputs

B Liu, NS Sartorio, RG Izzard… - Monthly Notices of the …, 2024 - academic.oup.com
ABSTRACT X-ray binaries (XRBs) are thought to regulate cosmic thermal and ionization
histories during the Epoch of Reionization and Cosmic Dawn (z∼ 5–30). Theoretical …

The CHARA Array interferometric program on the multiplicity of classical Be stars: new detections and orbits of stripped subdwarf companions

R Klement, T Rivinius, DR Gies, D Baade… - The Astrophysical …, 2024 - iopscience.iop.org
Rapid rotation and nonradial pulsations enable Be stars to build decretion disks, where the
characteristic line emission forms. A major but unconstrained fraction of Be stars owe their …

VLA monitoring of LS V+ 44 17 reveals scatter in the X-ray–radio correlation of Be/X-ray binaries

J Van den Eijnden, A Rouco Escorial… - Monthly Notices of …, 2024 - academic.oup.com
ABSTRACT LS V+ 44 17 is a persistent Be/X-ray binary (BeXRB) that displayed a bright,
double-peaked period of X-ray activity in late 2022/early 2023. We present a radio …

Verification of Astrometrically Accelerating Stars from Hipparcos and Gaia. I. Methodology and Application to HIP 44842

VV Makarov, A Tokovinin - The Astronomical Journal, 2024 - iopscience.iop.org
A large number of candidate binary stars with apparent acceleration on the sky has emerged
from analysis of astrometric data collected by the Hipparcos, Tycho-2, and Gaia space …

To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries

KA Rocha, V Kalogera, Z Doctor, JJ Andrews… - arXiv preprint arXiv …, 2024 - arxiv.org
Be X-ray binaries (Be-XRBs) are crucial in understanding high-mass X-ray binaries,
featuring a rapidly rotating Be star and a neutron star companion in an eccentric orbit …

A Sample of Compact Object Candidates in Single-lined Spectroscopic Binaries from LAMOST Medium Resolution Survey

HB Liu, WM Gu, ZX Zhang, T Yi, JZ Liu… - arXiv preprint arXiv …, 2024 - arxiv.org
The stellar spectra from LAMOST Medium Resolution Survey can be used to search for
compact objects in binaries. The LAMOST DR10 catalog includes> 980, 000 targets with …

The nature of the accretion physics in quiescent black hole system LB-1

T Su, E Qiao, S Wang - arXiv preprint arXiv:2406.09064, 2024 - arxiv.org
LB-1 is a binary system that has drawn great attention since its discovery in 2019. The
nature of the two components of LB-1 is not very clear, which however is suggested very …

Using SMC OB Field Stars and Field Binaries to Study the Origin and Evolution of Massive Star Populations

S Oey, FC Adams, J Eldridge, LW Hartmann - 2024 - deepblue.lib.umich.edu
Massive field stars are a seemingly isolated population that can be used to probe massive
star formation, binary interactions and massive star evolution. Field stars typically comprise …