Cover Image

Irradiation-Driven Formation of Supersoft X-ray Sources Following Classical Novae

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	Zhao, Weitao, Meng, Xiangcun, Cui, Yingzhen, Guo, Yunlang
Format:	Preprint
Published:	2025
Subjects:	High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Similar Items

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

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

Irradiation effect and binary radio pulsars with giant companions
by: Lan, Shunyi, et al.
Published: (2024)

Spectral Energy Distribution Analysis of the Supersoft X-ray Source CAL 87: Multiwavelength Constraints
by: Stecchini, Paulo E., et al.
Published: (2025)

[HP99] 159 -- Properties of the first Supersoft X-ray Source with a Helium star donor
by: Szegedi, Hélène, et al.
Published: (2026)

Eccentric millisecond pulsar + subdwarf B star from rotationally delayed accretion-induced-collapse scenario
by: Meng, Xiangcun
Published: (2025)

The Formation of Electron-capture Supernovae: A Review
by: Wang, Bo, et al.
Published: (2025)

Ultra-compact X-ray Binaries: A Review
by: Wang, Bo, et al.
Published: (2026)

Ultraluminous X-ray sources with He star companions
by: Li, Luhan, et al.
Published: (2024)

Impact of convective overshooting on the single-degenerate model of Type Ia supernovae
by: Wang, Xinghuan, et al.
Published: (2025)

Formation of millisecond pulsars with wide orbits
by: Wang, Bo, et al.
Published: (2024)

Producing type Ia supernovae from hybrid CONe white dwarfs with main-sequence binary companions at low metallicity of Z = 0.0001
by: Guo, Boyang, et al.
Published: (2025)

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

Formation of black holes from He stars
by: Long, Gang, et al.
Published: (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
by: Starrfield, S., et al.
Published: (2025)

Eclipsing millisecond pulsars with He star companions
by: Guo, Yunlang, et al.
Published: (2025)

Deep Adaptive Optics Imaging Rules Out a Helium Star Companion to PSR J1928+1815
by: Nagarajan, Pranav, et al.
Published: (2026)

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

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

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

A Comprehensive Analysis of X-ray Sources in Terzan 5 Using Chandra Observations
by: Kumawat, Gourav, et al.
Published: (2025)

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

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

Formation of Wind-Fed Black Hole High-mass X-ray Binaries: The Role of Roche-lobe-Overflow Post Black-Hole Formation
by: Xing, Zepei, et al.
Published: (2024)

Height and Energy Evolution of X-ray Double Sources in a Solar Flare
by: Pan, Hanya, et al.
Published: (2025)

Rethinking Thorne-Żytkow Object Formation: The Fate of X-ray Binary LMC X-4 and Implications for Ultra-long Gamma-ray Bursts
by: Hutchinson-Smith, Tenley, et al.
Published: (2023)

Transient X-ray Sources as Extremely Eccentric Mass-Transfer Binaries with Compact Companions
by: Katz, Jonathan I., et al.
Published: (2026)

Formation of a Possible Black-hole Ultracompact X-ray Binary with the Shortest Orbital Period
by: Yang, Xing-Peng, et al.
Published: (2025)

X-ray Polarimetry of X-ray Pulsars
by: Poutanen, Juri, et al.
Published: (2024)

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

Orbital-period Changes of Low-mass X-ray Binaries Driven by Magnetic Braking
by: Fan, Yun-Ning, et al.
Published: (2024)

A Multiwavelength View of $ρ$ Oph I: Resolving the X-ray Source Between A and B
by: Gunderson, Sean J., et al.
Published: (2025)

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

To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries
by: Rocha, Kyle Akira, et al.
Published: (2024)

A potential mass-gap black hole in a wide binary with a circular orbit
by: Song, Wang, et al.
Published: (2024)

A Statistical Study of Soft X-ray Flares on Solar-type Stars
by: Zhao, Zhanhao, et al.
Published: (2023)

NICER observations of type-I X-ray bursts from the ultra-compact X-ray binary M15 X-2
by: Teodori, María Alejandra Díaz, et al.
Published: (2025)

Birthplaces of X-ray emission lines in Cygnus X-3
by: Vilhu, Osmi, et al.
Published: (2025)

X-ray spectropolarimetry of the bright atoll Serpens X-1
by: Ursini, F., et al.
Published: (2024)

Localizing short-period pulsations in hard X-rays and Gamma-rays during an X9.0 flare
by: Li, Dong
Published: (2025)