Imagen de Portada

Interacting binaries on the Main Sequence as in-situ tracers of mass transfer efficiency and stability

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Sen, Koushik, Renzo, Mathieu, Jin, Harim, Langer, Norbert, Schootemeijer, Abel, Villaseñor, Jaime I., Mahy, Laurent, Grichener, Aldana, Shah, Neev, Wang, Chen, Xu, Xiao-Tian
Formato:	Preprint
Publicado:	2025
Materias:	Solar and Stellar Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Unraveling the Origin of Unequal Mass Gravitational Wave Events: Insights from a Galactic High Mass X-ray Binary
por: Shah, Neev, et al.
Publicado: (2026)

The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
por: Ercolino, Andrea, et al.
Publicado: (2025)

Analytic approximations for massive close post-mass transfer binary systems
por: Schürmann, Christoph, et al.
Publicado: (2024)

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

A comprehensive grid of massive binary evolution models for the Galaxy - Surface properties of post-mass transfer stars
por: Jin, Harim, et al.
Publicado: (2025)

Mergers of compact objects with cores of massive stars: evolutionary pathways, r-process nucleosynthesis and multi-messenger signatures
por: Grichener, Aldana
Publicado: (2024)

Circumbinary disks in post common envelope binary systems with compact objects
por: Unger, Lotem, et al.
Publicado: (2024)

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models
por: Ercolino, Andrea, et al.
Publicado: (2026)

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

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

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

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

A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
por: Schootemeijer, Abel, et al.
Publicado: (2025)

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

A sequence of Type Ib, IIb, II-L, and II-P supernovae from binary-star progenitors of varying initial separation
por: Dessart, Luc, et al.
Publicado: (2024)

Massive stars in metal-poor dwarf galaxies are often extreme rotators
por: Schootemeijer, Abel, et al.
Publicado: (2022)

Basic stellar observables
por: Mahy, Laurent
Publicado: (2024)

The physical properties of post-mass-transfer binaries
por: Seeburger, Rhys, et al.
Publicado: (2025)

An absence of binary companions to Wolf-Rayet stars in the Small Magellanic Cloud: implications for mass loss and black hole masses at low metallicity
por: Schootemeijer, A., et al.
Publicado: (2024)

Evolution of wide O star binaries through their LBV stage. Population synthesis with mass-ejection-driven orbital evolution
por: Xu, Xiao-Tian, et al.
Publicado: (2026)

Stripped helium-star and compact object binaries in coeval populations -- predictions based on detailed binary evolution models
por: Wang, Chen, et al.
Publicado: (2024)

Constraining the overcontact phase in massive binary evolution -- III. Period stability of known B+B and O+B overcontact systems
por: Vrancken, Jasmine, et al.
Publicado: (2024)

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

Dataset for ''Optimal work control for an activity-driven odd tracer in a viscoelastic bath"
por: Goswami, Koushik
Publicado: (2026)

Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
por: Jin, Harim, et al.
Publicado: (2024)

Low-mass stellar and substellar candidate companions around massive stars in Sco OB1 and M17
por: Pauwels, Tinne, et al.
Publicado: (2024)

The mass distribution of stars stripped in binaries: The effect of metallicity
por: Hovis-Afflerbach, B., et al.
Publicado: (2024)

A chemically peculiar Be-shell star in a sub-solar metallicity solution for the post-mass-transfer eclipsing binary V658 Car
por: Hauck, Norbert
Publicado: (2026)

Main-sequence systems: orbital stability in stellar binaries
por: Quarles, Billy, et al.
Publicado: (2024)

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

Progenitor with small reaction networks should not be used as initial conditions for core collapse
por: Renzo, M., et al.
Publicado: (2024)

KISS Sorcar: A Stupidly-Simple General-Purpose and Software Engineering AI Assistant
por: Sen, Koushik
Publicado: (2026)

X-ray emission from helium star+black hole binaries as probes of tidally induced spin-up of second-born black holes
por: Sen, Koushik, et al.
Publicado: (2025)

Whispering in the dark: Faint X-ray emission from black holes with OB star companions
por: Sen, Koushik, et al.
Publicado: (2024)

From spatial to null infinity: Connecting initial data to peeling
por: Schneider, Berend, et al.
Publicado: (2025)

Unified Treatment of null and Spatial Infinity IV: Angular Momentum at Null and Spatial Infinity
por: Ashtekar, Abhay, et al.
Publicado: (2023)

Unified Treatment of Null and Spatial Infinity III: Asymptotically Minkowski Space-times
por: Ashtekar, Abhay, et al.
Publicado: (2023)

On the effects of radiation on mass transfer in binary stars
por: Cehula, Jakub, et al.
Publicado: (2025)

Nuclear Neural Networks: Emulating Late Burning Stages in Core Collapse Supernova Progenitors
por: Grichener, Aldana, et al.
Publicado: (2025)

The IACOB project XIII. Helium enrichment in O-type stars as a tracer of past binary interaction
por: Martínez-Sebastián, C., et al.
Publicado: (2024)