Copertina

Recurrent Nova V2487 Oph Had Superflares in 1941 and 1942 With Radiant Energies 10$^{42.5\pm1.6}$ Ergs

Fuente: arXiv

Salvato in:

Dettagli Bibliografici
Autore principale:	Schaefer, Bradley E.
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	Solar and Stellar Astrophysics High Energy Astrophysical Phenomena
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi

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

Orbital Period Changes of Recurrent Nova T Pyxidis Demonstrate that M_ejecta >> 11.3xM_accreted and Is Not a Type Ia Supernova Progenitor
di: Schaefer, Bradley E.
Pubblicazione: (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
di: Schaefer, Bradley E.
Pubblicazione: (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
di: Schaefer, Bradley E., et al.
Pubblicazione: (2025)

Evolutionary Period Changes for 25 X-ray Binaries and the Measurement of an Empirical Universal Law for Angular Momentum Loss in Accreting Binaries
di: Schaefer, Bradley E.
Pubblicazione: (2025)

Characterizing Superflares in HR 1099 using Temporal and Spectral Analysis of XMM-Newton Observations
di: Didel, Shweta, et al.
Pubblicazione: (2024)

Symbiotic Stars (Including T Corona Borealis) Are Not Immediate Progenitors of Normal Type Ia Supernovae
di: Schaefer, Bradley E.
Pubblicazione: (2025)

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

Multi-wavelength Study of A Superflare on RS CVn-type Star HD22468 Triggered at Hard X-ray by SVOM
di: Wang, J., et al.
Pubblicazione: (2026)

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

Detection of RS Oph with LST-1 and modelling of its HE/VHE gamma-ray emission
di: Project, CTA-LST, et al.
Pubblicazione: (2025)

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

New Approach to Superflare Energy Determination
di: Heinzel, Petr, et al.
Pubblicazione: (2026)

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

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

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

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

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

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

Comprehensive Listing of 208 Nova White Dwarf Masses As the Primary Determinant of Spectral-Class and Light-Curve-Class
di: Schaefer, Bradley E.
Pubblicazione: (2025)

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

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

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

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

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

The core collapse of a 16.5 M$_{\odot}$ star
di: Aryan, Amar, et al.
Pubblicazione: (2024)

A Minimal Interpretation of the Galactic Cosmic-Ray Proton and Helium Spectra from GeV to PeV Energies
di: Aharonian, Felix, et al.
Pubblicazione: (2026)

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

Multidimensional Nova Simulations with an Extended Buffer and Lower Initial Mixing Temperatures
di: Clark, Alexander Smith, et al.
Pubblicazione: (2025)

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

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

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

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

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

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

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

Reconstructing the mid-infrared environment in the stellar merger remnant V838 Monocerotis
di: Mobeen, Muhammad Zain, et al.
Pubblicazione: (2023)

Hydrodynamic Evolution and Detectability of Nova Remnants in the Galactic Center
di: Su, Zhao, et al.
Pubblicazione: (2025)

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

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