Cover Image

Multidimensional Nova Simulations with an Extended Buffer and Lower Initial Mixing Temperatures

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	Clark, Alexander Smith, Zingale, Michael
Format:	Preprint
Published:	2025
Subjects:	Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Similar Items

Sensitivity of 3D Convective Urca Simulations to Changes in Urca Reactions
by: Boyd, Brendan, et al.
Published: (2023)

Sensitivity of Simulations of Double Detonation Type Ia Supernova to Integration Methodology
by: Zingale, Michael, et al.
Published: (2023)

Numerical Treatment of Shock-Induced Nuclear Burning in Double Detonation Type Ia Supernovae
by: Brady, Ryan, et al.
Published: (2025)

Strong Coupling of Hydrodynamics and Reactions in Nuclear Statistical Equilibrium for Modeling Convection in Massive Stars
by: Zingale, Michael, et al.
Published: (2024)

3D Convective Urca Process in a Simmering White Dwarf
by: Boyd, Brendan, et al.
Published: (2024)

Multidimensional Radiation Hydrodynamics Simulations of Supernova 1987A Shock Breakout
by: Chen, Wun-Yi, et al.
Published: (2024)

Two-Dimensional Radiation-Hydrodynamic Simulations of Luminous Red Novae
by: Kirilov, Anthony, et al.
Published: (2025)

Suppression of Shock X-ray Emission in Novae from Turbulent Mixing with Cool Gas
by: Metzger, Brian D., et al.
Published: (2025)

Moving-Mesh Simulations of Mini-Common Envelope Ejection in Classical Novae
by: Nelson, Nicholas, et al.
Published: (2026)

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

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

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

Impacts of Multidimensional Progenitor Perturbations on Core-Collapse Supernova Explosions
by: Chen, Chien-Hui, et al.
Published: (2026)

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

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

The Accelerating Decline of the Mass Transfer Rate in the Recurrent Nova T Pyxidis
by: Godon, P., et al.
Published: (2024)

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

Irradiation-Driven Formation of Supersoft X-ray Sources Following Classical Novae
by: Zhao, Weitao, et al.
Published: (2025)

Simulating super-Chandrasekhar white dwarfs
by: Zuraiq, Zenia, et al.
Published: (2024)

An X-ray and Optical Study of the Dwarf Nova Candidate OGLE-BLG-DN-0064
by: Sibgatullin, A. B., et al.
Published: (2025)

Multidimensional Nebular-Phase Calculations of Dynamically-Driven Double-Degenerate Double-Detonation Models for Type Ia Supernovae
by: Pollin, J. M., et al.
Published: (2025)

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

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

True Unicorns and False Positives: Simulated Probabilities of Dark Massive Companions to Bright Stars
by: Miller, Andrew M., et al.
Published: (2024)

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

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

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

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

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

Millinovae: A New Class of Transient Supersoft X-ray Sources without a Classical Nova Eruption
by: Mróz, Przemek, et al.
Published: (2024)

Nucleosynthesis in Type Ia Supernovae, Classical Novae, and Type I X-Ray Bursts. A Primer on Stellar Explosions
by: Jose, Jordi
Published: (2026)

A morphological catalogue of Nova Remnants
by: Santamaria, Edgar, et al.
Published: (2025)

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

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

Revisiting the Classics: On the Statistics of Dust Formation in Novae
by: Chong, Atticus, et al.
Published: (2025)

A New WZ Sagittae-type Dwarf Nova KSP-OT-202104a Near the Period Minimum from the KMTNet Supernova Program
by: Kim, Sang Chul, et al.
Published: (2026)

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

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

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

Luminous Blue Variables
by: Smith, Nathan
Published: (2025)