Fermi-bubble bulk and edge analysis reveals dust, cooling breaks, and cosmic-ray diffusion, facilitating a self-consistent model
Fuente:
arXiv
Guardado en:
| Autores principales: | Keshet, Uri, Gurwich, Ilya, Lavi, Assaf, Avitan, Dina, Linnik, Teodor |
|---|---|
| Formato: | Preprint |
| Publicado: |
2023
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Detection of polarized Fermi-bubble synchrotron and dust emission
por: Keshet, Uri
Publicado: (2024)
por: Keshet, Uri
Publicado: (2024)
Mach $>3$ shocks at the tips of both eROSITA bubbles
por: Keshet, Uri, et al.
Publicado: (2026)
por: Keshet, Uri, et al.
Publicado: (2026)
Nested Fermi and eROSITA bubbles require very similar $\sim10^{56}$ erg collimated Galactic-center outbursts; their asymmetry indicates an eastern density gradient
por: Ghosh, Arka, et al.
Publicado: (2026)
por: Ghosh, Arka, et al.
Publicado: (2026)
Galaxy-cluster-stacked Fermi-LAT II: extended central hadronic signal
por: Keshet, Uri
Publicado: (2025)
por: Keshet, Uri
Publicado: (2025)
Galaxy-cluster-stacked Fermi-LAT III: substructure and radio-relic counterparts
por: Keshet, Uri
Publicado: (2025)
por: Keshet, Uri
Publicado: (2025)
Radially polarized synchrotron from galaxy-cluster virial shocks
por: Keshet, Uri
Publicado: (2024)
por: Keshet, Uri
Publicado: (2024)
Coma cluster $γ$-ray and radio emission is consistent with a secondary electron origin for the radio halo
por: Kushnir, Doron, et al.
Publicado: (2024)
por: Kushnir, Doron, et al.
Publicado: (2024)
Relativistic ions with power-law spectra explain radio phoenixes
por: Keshet, Uri
Publicado: (2025)
por: Keshet, Uri
Publicado: (2025)
Spatial dependence of the break in the energy spectrum of cosmic rays in the new anisotropic diffusion approach
por: Borisov, Vladislav, et al.
Publicado: (2025)
por: Borisov, Vladislav, et al.
Publicado: (2025)
Excess cataloged X-ray and radio sources at galaxy-cluster virial shocks
por: Ilani, Gideon, et al.
Publicado: (2024)
por: Ilani, Gideon, et al.
Publicado: (2024)
Contribution of the Cygnus bubble to the Galactic cosmic ray spectrum and diffuse $γ$-ray emissions
por: Nie, Lin, et al.
Publicado: (2024)
por: Nie, Lin, et al.
Publicado: (2024)
Interstellar dust revealed by light from cosmic dawn
por: Yang, Xuejuan, et al.
Publicado: (2025)
por: Yang, Xuejuan, et al.
Publicado: (2025)
Vertical shear instability with dust evolution and consistent cooling times. On the importance of the initial dust distribution
por: Pfeil, Thomas, et al.
Publicado: (2024)
por: Pfeil, Thomas, et al.
Publicado: (2024)
The distribution of misalignment angles in multipolar planetary nebulae
por: Avitan, Ido, et al.
Publicado: (2025)
por: Avitan, Ido, et al.
Publicado: (2025)
Cosmic rays, gas and dust in the Central Molecular Zone I -- $X_{CO}$ factors, cosmic-ray densities and dust opacities
por: Ren, H. X., et al.
Publicado: (2025)
por: Ren, H. X., et al.
Publicado: (2025)
A self-consistent model for dust settling and the vertical shear instability in protoplanetary disks
por: Fukuhara, Yuya, et al.
Publicado: (2024)
por: Fukuhara, Yuya, et al.
Publicado: (2024)
Cavitation instability in unmagnetized relativistic pair shocks
por: Demidov, Ivan, et al.
Publicado: (2025)
por: Demidov, Ivan, et al.
Publicado: (2025)
Macroscopic magnetization of primordial plasma by virial shocks
por: Keshet, Uri, et al.
Publicado: (2024)
por: Keshet, Uri, et al.
Publicado: (2024)
Stellar wind bubbles of OB stars as Galactic cosmic-ray re-accelerators
por: Meyer, Dominique M. -A.
Publicado: (2024)
por: Meyer, Dominique M. -A.
Publicado: (2024)
Galaxy cluster virial-shock sources in eROSITA catalogs
por: Ilani, Gideon, et al.
Publicado: (2024)
por: Ilani, Gideon, et al.
Publicado: (2024)
Propagation of Galactic cosmic rays: the influence of anisotropic diffusion
por: AL-Zetoun, Ala'a
Publicado: (2025)
por: AL-Zetoun, Ala'a
Publicado: (2025)
Effective cosmic ray diffusion in multiphase galactic environments
por: Thomas, Timon, et al.
Publicado: (2025)
por: Thomas, Timon, et al.
Publicado: (2025)
Supernova remnants in super bubbles as cosmic ray accelerators
por: Sushch, Iurii, et al.
Publicado: (2025)
por: Sushch, Iurii, et al.
Publicado: (2025)
Is cosmic dust porous?
por: Potapov, Alexey, et al.
Publicado: (2025)
por: Potapov, Alexey, et al.
Publicado: (2025)
The impact of cosmic ray heating on the cooling of the low-metallicity interstellar medium
por: Brugaletta, Vittoria, et al.
Publicado: (2024)
por: Brugaletta, Vittoria, et al.
Publicado: (2024)
Stochastic modelling of cosmic-ray sources for Galactic diffuse emissions
por: Stall, Anton, et al.
Publicado: (2025)
por: Stall, Anton, et al.
Publicado: (2025)
Dust formation in common envelope binary interactions -- II: 3D simulations with self-consistent dust formation
por: Bermúdez-Bustamante, Luis C., et al.
Publicado: (2024)
por: Bermúdez-Bustamante, Luis C., et al.
Publicado: (2024)
Self-consistent model of cosmic ray penetration into molecular clouds: Effect of energy losses
por: Chernyshov, D. O., et al.
Publicado: (2025)
por: Chernyshov, D. O., et al.
Publicado: (2025)
The MAGPI Survey: Insights into the Lyman-alpha line widths and the size of ionized bubbles at the edge of cosmic reionization
por: Mukherjee, T., et al.
Publicado: (2024)
por: Mukherjee, T., et al.
Publicado: (2024)
The cosmic journey of dust grains -- from nucleation to planetary system
por: Lund, Kira, et al.
Publicado: (2025)
por: Lund, Kira, et al.
Publicado: (2025)
The impact of the eROSITA bubbles on Galactic cosmic-ray transport
por: Schroer, Benedikt
Publicado: (2026)
por: Schroer, Benedikt
Publicado: (2026)
A grid of self-consistent MSG (MARCS-StaticWeather-GGchem) cool stellar, sub-stellar, and exoplanetary model atmospheres
por: Jørgensen, Uffe G., et al.
Publicado: (2024)
por: Jørgensen, Uffe G., et al.
Publicado: (2024)
THEMIS 2.0: A self-consistent model for dust extinction, emission, and polarisation
por: Ysard, Nathalie, et al.
Publicado: (2024)
por: Ysard, Nathalie, et al.
Publicado: (2024)
Hydrodynamic model of nonthermal emission from the Fermi bubbles
por: Dogiel, V. A., et al.
Publicado: (2026)
por: Dogiel, V. A., et al.
Publicado: (2026)
Simulating cosmic ray electron spectra and radio emission from an AGN jet outburst in a cool-core cluster
por: Jlassi, Léna, et al.
Publicado: (2026)
por: Jlassi, Léna, et al.
Publicado: (2026)
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)
por: Martí-Devesa, G., et al.
Publicado: (2024)
Tidal disruption events as the origin of the eROSITA and Fermi bubbles
por: Scheffler, Tassilo, et al.
Publicado: (2025)
por: Scheffler, Tassilo, et al.
Publicado: (2025)
Search for cosmic-ray induced gamma-ray emission from local galaxy clusters using Fermi-LAT data
por: Pérez-Romero, Judit, et al.
Publicado: (2025)
por: Pérez-Romero, Judit, et al.
Publicado: (2025)
Re-evaluation of the cosmic-ray ionization rate in diffuse clouds
por: Obolentseva, M., et al.
Publicado: (2024)
por: Obolentseva, M., et al.
Publicado: (2024)
Formation of dust grains in the winds of cool giants, PhD thesis 1992
por: Dominik, C.
Publicado: (2026)
por: Dominik, C.
Publicado: (2026)
Ejemplares similares
-
Detection of polarized Fermi-bubble synchrotron and dust emission
por: Keshet, Uri
Publicado: (2024) -
Mach $>3$ shocks at the tips of both eROSITA bubbles
por: Keshet, Uri, et al.
Publicado: (2026) -
Nested Fermi and eROSITA bubbles require very similar $\sim10^{56}$ erg collimated Galactic-center outbursts; their asymmetry indicates an eastern density gradient
por: Ghosh, Arka, et al.
Publicado: (2026) -
Galaxy-cluster-stacked Fermi-LAT II: extended central hadronic signal
por: Keshet, Uri
Publicado: (2025) -
Galaxy-cluster-stacked Fermi-LAT III: substructure and radio-relic counterparts
por: Keshet, Uri
Publicado: (2025)