Imagen de Portada

Exploring mass transfer mechanisms in symbiotic systems

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Vathachira, Irin Babu, Hillman, Yael, Kashi, Amit
Formato:	Preprint
Publicado:	2025
Materias:	Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

The Role of Binary Configuration in Shaping Nova Evolution via Wind Accretion in Symbiotic Systems
por: Vathachira, Irin Babu, et al.
Publicado: (2025)

Accretion and Recovery in Giant Eruptions of Massive Stars
por: Mukhija, Bhawna, et al.
Publicado: (2025)

Wind Accretion in Massive Binaries Experiencing High Mass Loss Rates: I. Dependency on Mass Ratio and Orbital Period
por: Mukhija, Bhawna, et al.
Publicado: (2025)

High Power Accretion in Massive Binary Systems and the Impact of Metallicity
por: Mukhija, Bhawna, et al.
Publicado: (2025)

Wind Accretion in Massive Binaries Experiencing High Mass Loss Rates: II. Eccentricity
por: Mukhija, Bhawna, et al.
Publicado: (2026)

It's always the quiet ones: Single Degenerate Double Detonation Type Ia Supernova from Quiescent Helium Accretion
por: Michaelis, Amir, et al.
Publicado: (2025)

Helium Accumulation and Thermonuclear Instabilities on Accreting White Dwarfs: From Recurring Helium Novae to Type Ia Supernovae
por: Hillman, Yael, et al.
Publicado: (2025)

HD3191, the high-mass X-ray binary that wasn't there
por: Rauw, Gregor, et al.
Publicado: (2026)

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

Interacting supernovae from wide mass-transferring binaries
por: Ercolino, Andrea
Publicado: (2024)

Understanding the impact of binary mass transfer in the accretor's measurable parameters
por: Vilaxa-Campos, Magdalena, et al.
Publicado: (2026)

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

WR + O binaries as probes of the first phase of mass transfer
por: Nuijten, Marit, et al.
Publicado: (2024)

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

Binary mass transfer in 3D: Mass Transfer Rate and Morphology
por: Ryu, T., et al.
Publicado: (2025)

Rapid binary mass transfer: Circumbinary outflows and angular momentum losses
por: Scherbak, Peter, et al.
Publicado: (2025)

Expansion of accreting main-sequence stars during rapid mass transfer
por: Lau, Mike Y. M., et al.
Publicado: (2024)

Ancient nova shells of RX Pup indicate evolution of mass transfer rate
por: Ilkiewicz, Krystian, et al.
Publicado: (2024)

Y Gem, a symbiotic star outshone by its asymptotic giant branch primary component
por: Guerrero, M. A., et al.
Publicado: (2024)

An optical--mid-infrared color evolution tool for nova identification using WISE data
por: Onuegbu, Joseph, et al.
Publicado: (2025)

X-raying the zeta Tau binary system
por: Naze, Yael, et al.
Publicado: (2024)

Another one (BH+OB pair) bites the dust
por: Naze, Yael, et al.
Publicado: (2025)

Irradiation-driven mass transfer for massive companion stars in supersoft X-rays sources
por: Zhao, Weitao, et al.
Publicado: (2024)

Coping with loss: Stability of mass transfer from post-main sequence donor stars
por: Temmink, K. D., et al.
Publicado: (2022)

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)

CGCS 6306, another X-ray-emitting asymptotic giant branch star confirmed to be a symbiotic binary
por: Merc, Jaroslav, et al.
Publicado: (2025)

The symbiotic star V694 Mon has transitioned from the accreting-only state to the steady burning phase
por: Munari, Ulisse
Publicado: (2024)

Modeling the high-brightness state of the recurrent nova T CrB as an enhanced mass-transfer event
por: Schlindwein, Wagner, et al.
Publicado: (2025)

Expanding the ultracompacts: gravitational wave-driven mass transfer in the shortest-period binaries with accretion disks
por: Chakraborty, Joheen, et al.
Publicado: (2024)

The slowest spinning Galactic-field spider PSR J1932+2121: A history of inefficient mass transfer
por: Misra, Devina, et al.
Publicado: (2025)

Population synthesis of Be X-ray binaries in the Small Magellanic Cloud: angular momentum recycling and stable mass transfer
por: Oller, Víctor López, et al.
Publicado: (2026)

Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
por: Schneider, F. R. N., et al.
Publicado: (2025)

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

X-raying the wind-wind collisions in HD 168112 and HD 167971
por: Rauw, Gregor, et al.
Publicado: (2024)

Evolution of neutron stars in wide eccentric low-mass binary systems
por: Afonina, Marina, et al.
Publicado: (2025)

A new way to find symbiotic stars: accretion disc detection with continuum survey photometry
por: Lucy, A. B., et al.
Publicado: (2024)

Orbital motion detected in gamma Cas Fe K emission lines
por: Naze, Yael, et al.
Publicado: (2026)

High-resolution imaging of the evolving bipolar outflows in symbiotic novae: The case of the RSOphiuchi 2021 nova outburst
por: Lico, R., et al.
Publicado: (2024)

Exploring extreme brightness variations in blue supergiant MACHO 80.7443.1718: Evidence for companion-driven enhanced mass loss
por: Kołaczek-Szymański, Piotr Antoni, et al.
Publicado: (2023)

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