Imagen de Portada

Predicting the next local supernova

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autor principal:	Middleditch, John
Formato:	Preprint
Publicado:	2019
Materias:	High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Disruption of Supernovae and would-be "Direct Collapsars"
por: Middleditch, John
Publicado: (2019)

The next galactic supernova can uncover mass and couplings of particles decaying to neutrinos
por: Telalovic, Bernanda, et al.
Publicado: (2024)

Neutrino flux sensitivity to the next galactic core-collapse supernova in COSINUS
por: Angloher, G., et al.
Publicado: (2024)

IXPE observations of supernova remnants
por: Ferrazzoli, Riccardo
Publicado: (2025)

Looking into the world of interacting supernovae
por: Gangopadhyay, Anjasha
Publicado: (2024)

Comprehensive neutrino light curves and spectra: from pre-supernova evolution to early supernova phase
por: Kato, Chinami, et al.
Publicado: (2026)

On the properties of turbulence in the remnant of Tycho supernova
por: Petruk, Oleh, et al.
Publicado: (2025)

Interacting supernovae and where to find them
por: Brose, Robert, et al.
Publicado: (2025)

Probing supernovae and kicks in post-supernova binaries
por: Larsen, Claudia, et al.
Publicado: (2024)

Diffuse supernova neutrino background with up-to-date star formation rate measurements and long-term multidimensional supernova simulations
por: Ekanger, Nick, et al.
Publicado: (2023)

Regions of suppressed diffusion around supernova remnants?
por: Bao, Yiwei, et al.
Publicado: (2024)

Double shell structure in supernova 2024ggi
por: Shiran, Kobi, et al.
Publicado: (2025)

Particle acceleration at radiative supernova remnant shocks
por: Cristofari, Pierre
Publicado: (2025)

Pre-supernova outbursts by core magnetic activity
por: Cohen, Tamar, et al.
Publicado: (2023)

How do supernova remnants cool? II. Machine learning analysis of supernova remnant simulations
por: Smirnova, P., et al.
Publicado: (2024)

Inhomogeneous stellar mixing in the final hours before the Cassiopeia A supernova
por: Sato, Toshiki, et al.
Publicado: (2025)

Long-rising Type II supernovae resembling supernova 1987A -- II. A new analytical model to describe these events
por: Pumo, M. L., et al.
Publicado: (2025)

Explaining supernova remnant G352.7-0.1 as a peculiar type Ia supernova inside a planetary nebula
por: Soker, Noam
Publicado: (2024)

Interacting supernovae
por: Dessart, Luc
Publicado: (2024)

Type Ia supernova explosion models are inherently multidimensional
por: Pakmor, R., et al.
Publicado: (2024)

Gravitational wave radiation from magnetar-driven supernovae
por: Xie, Lang, et al.
Publicado: (2024)

Leveraging neutrino flavor physics for supernova model differentiation
por: Newkirk, Lily, et al.
Publicado: (2024)

Circular polarization of gravitational waves from magnetorotational supernovae
por: Shibagaki, Shota, et al.
Publicado: (2026)

Broadband radio study of the supernova remnant Kes 73
por: Loru, S., et al.
Publicado: (2025)

An investigation on the FWHM of absorption features of type Ia supernovae
por: Zhao, Xulin, et al.
Publicado: (2026)

Anisotropy of core-collapse supernovae effected by AGN disks
por: She, Jiao-Zhen, et al.
Publicado: (2025)

Nucleosynthesis in magnetorotational supernovae: impact of the magnetic field configuration
por: Reichert, M., et al.
Publicado: (2024)

The population of Galactic supernova remnants in the TeV range
por: Batzofin, Rowan, et al.
Publicado: (2024)

Diffusive shock acceleration of dust grains at supernova remnants
por: Cristofari, P., et al.
Publicado: (2024)

Type Ibn supernovae from ultra-stripped supernova progenitors
por: Moriya, Takashi J., et al.
Publicado: (2025)

Getting the most on supernova axions
por: Lella, Alessandro, et al.
Publicado: (2023)

On the formation of strange quark stars from supernova in compact binaries
por: Becerra, L. M., et al.
Publicado: (2025)

Evidence of gradients of density and magnetic field in the remnant of Tycho's supernova
por: Petruk, Oleh, et al.
Publicado: (2024)

On the acceleration of cosmic rays at the post-adiabatic shocks of supernova remnants
por: Petruk, O., et al.
Publicado: (2025)

The vela supernova remnant: The unique morphological features of jittering jets
por: Soker, Noam, et al.
Publicado: (2024)

Jittering jets promote dust formation in core-collapse supernovae
por: Soker, Noam
Publicado: (2025)

Broadband $γ$-ray spectrum of supernova remnant Cassiopeia A
por: Cao, Zhen, et al.
Publicado: (2025)

The precessing jet axis of the supernova remnant 3C 397
por: Klimov, Aleksei, et al.
Publicado: (2026)

Tycho supernova exploded inside a planetary nebula (SNIP)
por: Soker, Noam
Publicado: (2025)

Learning from core-collapse supernova remnants on the explosion mechanism
por: Soker, Noam
Publicado: (2024)