:: Library Catalog

Imagen de Portada

Guardado en:

Detalles Bibliográficos
Autores principales:	Godon, P., Sion, E. M., Williams, R. E., Darnley, M. J., Sokoloski, J. L., lawrence, S. S.
Formato:	Preprint
Publicado:	2024
Materias:	Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
Acceso en línea:	https://arxiv.org/abs/2409.02090
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Orbital Period Changes of Recurrent Nova T Pyxidis Demonstrate that M_ejecta >> 11.3xM_accreted and Is Not a Type Ia Supernova Progenitor
por: Schaefer, Bradley E.
Publicado: (2026)

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

Evolution of the recent high-accretion state of the recurrent nova T CrB: HST, Swift, NuSTAR, and XMM-Newton observations
por: Luna, G. J. M., et al.
Publicado: (2026)

Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It will be the Brightest Classical or Recurrent Nova Ever Observed in X-rays
por: Starrfield, S., et al.
Publicado: (2025)

Orbital Period Changes in Recurrent Nova T Corona Borealis Prove That It Is Not a Type Ia Supernovae Progenitor
por: Schaefer, Bradley E.
Publicado: (2025)

Association between Recurrent Novae and Nova Super-Remnants
por: Healy-Kalesh, Michael William
Publicado: (2024)

The Landscape of Unstable Mass Transfer in Interacting Binaries and Its Imprint on the Population of Luminous Red Novae
por: Twum, Angela A. G., et al.
Publicado: (2026)

A 70 pc-Diameter Nova Super-remnant Surrounding the Recurrent Nova RS Ophiuchi
por: Shara, Michael M., et al.
Publicado: (2025)

Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates
por: Scherbak, Peter, et al.
Publicado: (2025)

Recurrent Nova V2487 Oph Had Superflares in 1941 and 1942 With Radiant Energies 10$^{42.5\pm1.6}$ Ergs
por: Schaefer, Bradley E.
Publicado: (2024)

The Newly Discovered Nova Super-Remnant Surrounding Recurrent Nova T Coronae Borealis: Will it Light Up During the Coming Eruption?
por: Shara, Michael M., et al.
Publicado: (2024)

The Dusty Aftermath of a Rapid Nova: V5579 Sgr
por: Raj, A., et al.
Publicado: (2024)

Orbital Period Changes of Recurrent Nova U Scorpii Demonstrate that M$_{\rm ejecta}$=26$\times$M$_{\rm accreted}$ and Is Not a Type Ia Supernova Progenitor
por: Schaefer, Bradley E., et al.
Publicado: (2025)

Common Envelopes, Gamma Rays, and Sudden Spectral Changes of Novae
por: Williams, Robert, et al.
Publicado: (2024)

Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour
por: Merc, Jaroslav, et al.
Publicado: (2025)

Stellar Spin Down in Post-Mass Transfer Binary Systems
por: Sun, Meng, et al.
Publicado: (2024)

Ongoing and Post-Mass-Transfer Binaries: A Living Catalog and Unified Review of Binary Mass Transfer Products
por: van Son, Lieke A. C., et al.
Publicado: (2026)

The Rise of Nova V1674 Herculis
por: Quimby, Robert M., et al.
Publicado: (2024)

Discovery of Two New Eruptions of the Ultrashort Recurrence Time Nova M31N 2017-01e
por: Shafter, Allen W., et al.
Publicado: (2024)

Mass estimates from optical modelling of the new TRAPUM redback PSR J1910-5320
por: Dodge, O. G., et al.
Publicado: (2024)

Symbiotic stars in X-rays IV: XMM-Newton, Swift and TESS observations
por: Lima, Isabel J., et al.
Publicado: (2024)

Unified Rapid Mass Transfer
por: Ivanova, Natalia, et al.
Publicado: (2024)

Mass Transfer in Eccentric Orbits with Self-consistent Stellar Evolution
por: Rocha, Kyle Akira, et al.
Publicado: (2024)

Non-conservative Mass Transfer as a Formation Channel for Gaia Black Hole System
por: Olejak, Aleksandra, et al.
Publicado: (2025)

Challenging Classical Paradigms: Recurrent Nova M31N 2017-01e, a BeWD system in M31?
por: Chamoli, Shatakshi, et al.
Publicado: (2025)

Binarity Enhances the Occurrence Rate of Radiation Belt Emissions in Ultracool Dwarfs
por: Kao, Melodie M., et al.
Publicado: (2024)

A Catalogue of Ultracompact Mass-Transferring White Dwarf Binaries
por: Green, Matthew J., et al.
Publicado: (2025)

The Mass of the Vela Pulsar Progenitor and the Age of the Vela-Puppis Complex
por: Murphy, Jeremiah W., et al.
Publicado: (2024)

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)

The Unique Helium Nova V445 Puppis Ejected $\gg$0.001 M$_{\odot}$ in the Year 2000 and Will Not Become a Type Ia Supernova
por: Schaefer, Bradley E.
Publicado: (2024)

The physical properties of T Pyx as measured by MUSE I. The geometrical distribution of the ejecta and the distance to the remnant
por: Izzo, L., et al.
Publicado: (2023)

Constraining Lens Masses in Moderately to Highly Magnified Microlensing Events from Gaia
por: Pylypenko, U., et al.
Publicado: (2025)

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions
por: Lechien, Thibault, et al.
Publicado: (2025)

Correlating Particle Acceleration Rates with Plasma Conditions in Colliding Wind Binaries
por: Cordeiro, Gislaine B, et al.
Publicado: (2025)

Mass loss and the Eddington parameter
por: Bestenlehner, Joachim M.
Publicado: (2022)

X-Ray Flashes on Helium Novae
por: Kato, Mariko, et al.
Publicado: (2024)

Formation of Lower Mass-gap Black Hole--Neutron Star Binary Mergers through Super-Eddington Stable Mass Transfer
por: Zhu, Jin-Ping, et al.
Publicado: (2023)

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

Effect of Rotation on Wave Mixing in Intermediate Mass Stars
por: Varghese, A., et al.
Publicado: (2024)

Carbon-Oxygen Classical Novae are Galactic $^7$Li Producers as well as Potential Supernova Ia Progenitors
por: Starrfield, Sumner, et al.
Publicado: (2019)