Analytic approximations for massive close post-mass transfer binary systems

Fuente: arXiv

Salvato in:

Dettagli Bibliografici
Autori principali:	Schürmann, Christoph, Langer, Norbert, Kramer, Joana A., Marchant, Pablo, Wang, Chen, Sen, Koushik
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	Solar and Stellar Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi

Populations of evolved massive binary stars in the Small Magellanic Cloud I: Predictions from detailed evolution models
di: Xu, X. -T., et al.
Pubblicazione: (2025)

Evolution of binary stars
di: Marchant, Pablo
Pubblicazione: (2025)

Populations of evolved massive binary stars in the Small Magellanic Cloud II: Predictions from rapid binary evolution
di: Schürmann, C., et al.
Pubblicazione: (2025)

Radiation hydrodynamical simulations of super-Eddington mass transfer and black hole growth in close binaries
di: Toyouchi, Daisuke, et al.
Pubblicazione: (2024)

Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
di: Sciarini, Luca, et al.
Pubblicazione: (2026)

Exploring the borderline between stable mass transfer and mergers in close binary evolution
di: Schürmann, Christoph, et al.
Pubblicazione: (2024)

Interacting supernovae from wide massive binary systems
di: Ercolino, Andrea, et al.
Pubblicazione: (2023)

A fundamental limit to how close binary systems can get via stable mass transfer shapes the properties of binary black hole mergers
di: Klencki, Jakub, et al.
Pubblicazione: (2025)

A binary system in the S cluster close to the supermassive black hole Sagittarius A*
di: Peißker, Florian, et al.
Pubblicazione: (2024)

A new sample of massive B-type contact binary candidates from the OGLE survey of the Magellanic Clouds
di: Menon, Athira, et al.
Pubblicazione: (2024)

Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
di: Ma, Jing-Ze, et al.
Pubblicazione: (2025)

BH-BH mergers with & without EM counterpart: A model for stable tertiary mass transfer in hierarchical triple systems
di: Kummer, F., et al.
Pubblicazione: (2024)

An upper limit on the spins of merging binary black holes formed through binary evolution
di: Marchant, Pablo, et al.
Pubblicazione: (2023)

A new mass estimate method with hydrodynamical atmospheres for very massive WNh stars
di: Sabhahit, Gautham N., et al.
Pubblicazione: (2025)

Formation of massive multiple-star systems: early migration and mergers
di: Chon, Sunmyon, et al.
Pubblicazione: (2026)

Mass-transferring binary stars as progenitors of interacting hydrogen-free supernovae
di: Ercolino, Andrea, et al.
Pubblicazione: (2024)

Evolutionary tracks, ejecta, and ionizing photons from intermediate-mass to very massive stars with PARSEC
di: Costa, G., et al.
Pubblicazione: (2025)

Jet formation in post-AGB binaries: Confronting cold magnetohydrodynamic disc wind wind models with observations
di: De Prins, Toon, et al.
Pubblicazione: (2024)

Stable mass transfer in massive binaries leading to merging black holes
di: Xu, Xiao-Tian, et al.
Pubblicazione: (2025)

Two decades of optical variability of Small Magellanic Cloud high-mass X-ray binaries
di: Treiber, Helena, et al.
Pubblicazione: (2025)

Forming merging double compact objects with stable mass transfer
di: Picco, Annachiara, et al.
Pubblicazione: (2023)

The nebular spectra of SN 2023ixf: A lower mass, partially stripped progenitor may be the result of binary interaction
di: Michel, Philip D., et al.
Pubblicazione: (2025)

High mass function ellipsoidal variables in the Gaia Focused Product Release: searching for black hole candidates in the binary zoo
di: Rowan, D. M., et al.
Pubblicazione: (2024)

Searching for accreting compact binary systems from spectroscopy and photometry: Application to LAMOST spectra
di: Zhao, Xinlin, et al.
Pubblicazione: (2025)

Binarity at LOw Metallicity (BLOeM): Bayesian inference of natal kicks from inert black hole binaries
di: Willcox, R., et al.
Pubblicazione: (2025)

Spectacular nucleosynthesis from early massive stars
di: Ji, Alexander P., et al.
Pubblicazione: (2024)

The fate of rotating massive stars across cosmic times
di: Hirschi, R., et al.
Pubblicazione: (2025)

Gaia's binary star renaissance
di: El-Badry, Kareem
Pubblicazione: (2024)

Material mixing in pulsar wind nebulae of massive runaway stars
di: Meyer, D. M. -A., et al.
Pubblicazione: (2024)

Modeling contact binaries, III. Properties of a population of close, massive binaries
di: Fabry, Matthias, et al.
Pubblicazione: (2024)

Distinguishing between light curves of ellipsoidal variables with massive dark companions, contact binaries, and semidetached binaries using principal component analysis
di: Pešta, Milan, et al.
Pubblicazione: (2024)

Shells and bubbles around compact clusters of massive stars: 3D MHD simulations
di: Badmaev, D. V., et al.
Pubblicazione: (2026)

Two waves of massive stars running away from the young cluster R136
di: Stoop, Mitchel, et al.
Pubblicazione: (2024)

Discovery of a new transitional type of evolved massive stars with hard ionizing flux
di: Sander, Andreas A. C., et al.
Pubblicazione: (2025)

Radiative-transfer models for dusty Type II supernovae
di: Dessart, Luc, et al.
Pubblicazione: (2025)

SN 2017ati: A luminous type IIb explosion from a massive progenitor
di: Peng, Z. -H., et al.
Pubblicazione: (2026)

How interacting winds shape the mechanical feedback of massive star clusters over millions of years
di: Vieu, Thibault, et al.
Pubblicazione: (2026)

Detecting Detached Black Hole binaries through Photometric Variability
di: Chawla, Chirag, et al.
Pubblicazione: (2023)

SED and Galactic kinematic diagnostics for dormant BH/NS binary candidates
di: An, Qian-Yu, et al.
Pubblicazione: (2026)

Kinematic constraints on the ages and kick velocities of Galactic neutron star binaries
di: Disberg, Paul, et al.
Pubblicazione: (2024)