Imagen de Portada

X-ray polarization: A view deep inside cosmic ray driven turbulence and particle acceleration in supernova remnants

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Bykov, Andrei. M., Osipov, Sergei. M., Uvarov, Yury. A., Ellison, Donald. C., Slane, Patrick
Formato:	Preprint
Publicado:	2024
Materias:	High Energy Astrophysical Phenomena Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

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

PeV particle acceleration and non-thermal emission in the `minimalist' model of the extended jets in W50/SS433
por: Bykov, A. M., et al.
Publicado: (2025)

Investigating the CREDIT history of supernova remnants as cosmic-ray sources
por: Stall, Anton, et al.
Publicado: (2025)

Investigating the CREDIT history of supernova remnants as cosmic-ray sources
por: Stall, Anton, et al.
Publicado: (2024)

Cosmic ray acceleration and non-thermal emission from fast luminous optical transient sources
por: Romansky, V. I., et al.
Publicado: (2024)

Evidence of cosmic-ray acceleration up to sub-PeV energies in the supernova remnant IC 443
por: Cao, Zhen, et al.
Publicado: (2025)

Supernova remnants in super bubbles as cosmic ray accelerators
por: Sushch, Iurii, et al.
Publicado: (2025)

Ultra-high-energy $γ$-ray imprints from PeV particles accelerated by supernova remnants
por: Cao, Zhen, et al.
Publicado: (2026)

Infrared and X-ray emission of a supernova remnant in a clumpy medium
por: Dedikov, S. Yu., et al.
Publicado: (2025)

Hadronic particle acceleration in the supernova remnant SN 1006 as traced by Fermi-LAT observations
por: Lemoine-Goumard, M., et al.
Publicado: (2024)

Cosmic-ray acceleration and escape from supernova remnant W44 as probed by Fermi-LAT and MAGIC
por: Abe, S., et al.
Publicado: (2025)

Study of X-ray emission from the S147 nebula by SRG/eROSITA: supernova-in-the-cavity scenario
por: Khabibullin, Ildar I., et al.
Publicado: (2024)

Evidence for gamma-ray emission from the remnant of Kepler's supernova based on deep H.E.S.S. observations
por: Collaboration, H. E. S. S., et al.
Publicado: (2022)

TeV spectral bump of cosmic-ray protons and helium nuclei: the role of nearby supernova remnants
por: Bhadra, Sourav, et al.
Publicado: (2025)

Gamma radiation from cosmic rays escaping a young supernova remnant: The case of Cas A
por: Blasi, P.
Publicado: (2025)

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

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

Reinterpretation of the Fermi acceleration of cosmic rays in terms of the ballistic surfing acceleration in supernova shocks
por: Stasiewicz, Krzysztof
Publicado: (2024)

A second view on the X-ray polarization of NGC 4151 with IXPE
por: Gianolli, V. E., et al.
Publicado: (2024)

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

Evidence of polar and ultralow supernova kicks from the orbits of Be X-ray binaries
por: Valli, Ruggero, et al.
Publicado: (2025)

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

Microquasar remnants as reservoirs of PeV cosmic rays
por: Abaroa, Leandro, et al.
Publicado: (2026)

Dust destruction by the supernova remnant forward shock in a turbulent interstellar medium
por: Scheffler, Tassilo, et al.
Publicado: (2025)

Stellar wind bubbles of OB stars as Galactic cosmic-ray re-accelerators
por: Meyer, Dominique M. -A.
Publicado: (2024)

PeV proton acceleration in Gamma-ray Binaries
por: Bykov, A. M., et al.
Publicado: (2024)

Early-time gamma-ray constraints on cosmic-ray acceleration in the core-collapse SN 2023ixf with the Fermi Large Area Telescope
por: Martí-Devesa, G., et al.
Publicado: (2024)

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

Discovery of a shock-compressed magnetic field in the north-western rim of the young supernova remnant RX J1713.7-3946 with X-ray polarimetry
por: Ferrazzoli, Riccardo, et al.
Publicado: (2024)

Particle acceleration by turbulent-driven magnetic reconnection and the production of gamma-rays and neutrinos in AGNs
por: Pino, E. M. de Gouveia Dal, et al.
Publicado: (2025)

On the width of a collisionless shock and the index of the cosmic rays it accelerates
por: Bret, Antoine, et al.
Publicado: (2024)

Stellar energetic particle and cosmic ray effects in exoplanetary atmospheres
por: Rodgers-Lee, D.
Publicado: (2024)

Direct detection of the non-thermal X-ray emission from the Arches star cluster
por: Krivonos, Roman, et al.
Publicado: (2026)

X-ray diagnostics of Cassiopeia A's "Green Monster": evidence for dense shocked circumstellar plasma
por: Vink, Jacco, et al.
Publicado: (2024)

A fresh perspective on the 3D dynamics of Tycho's supernova remnant: Ejecta asymmetries in the X-ray band
por: Godinaud, Leila, et al.
Publicado: (2023)

Typing supernova remnant G352.7$-$0.1 using XMM-Newton X-ray observations
por: Dang, Ling-Xiao, et al.
Publicado: (2024)

Discovery of diffuse gamma-ray emission in the vicinity of G172.8+1.5: An old supernova remnant with different turbulence properties
por: Li, Yuan, et al.
Publicado: (2025)

Gamma rays as a signature of r-process producing supernovae: remnants and future Galactic explosions
por: Liu, Zhenghai, et al.
Publicado: (2025)

Radio signatures of cosmic-ray showers with deep in-ice antennas
por: Chiche, Simon, et al.
Publicado: (2024)

Magnetised turbulent plasmas as high-energy particle accelerators
por: Lemoine, M.
Publicado: (2025)