MHD decomposition explains diffuse <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>γ</mml:mi></mml:mrow></mml:math> -ray emission in Cygnus X

No abstract is available for this paper.

• Publication year

  2022

• Venue

  Physical Review D

• Publication date

  2022-11-15

• Fields of study

  Not labeled

• Identifiers
  DOI 10.1103/physrevd.106.103015
• External record

  Open on Semantic Scholar

• Source metadata

  Semantic Scholar

• No claims are published for this paper.

• No concepts are published for this paper.

• Ion alfvén velocity fluctuations and implications for the diffusion of streaming cosmic rays

  2022cited by this paper
• HAWC observations of the acceleration of very-high-energy cosmic rays in the Cygnus Cocoon

  2021cited by this paper
• Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 γ-ray Galactic sources

  2021cited by this paper
• Particle acceleration in winds of star clusters

  2021cited by this paper
• High-Energy Particles and Radiation in Star-Forming Regions

  2020cited by this paper
• The theory of cosmic ray scattering on pre-existing MHD modes meets data

  2020cited by this paper
• Massive stars as major factories of Galactic cosmic rays

  2018cited by this paper
• Identification of plasma modes in Galactic turbulence with synchrotron polarization

  2018cited by this paper
• Diffuse gamma-ray emission in the vicinity of young star cluster Westerlund 2

  2017cited by this paper
• Finite Difference Computing with PDEs

  2017cited by this paper
• SHOCKFIND - an algorithm to identify magnetohydrodynamic shock waves in turbulent clouds

  2016cited by this paper
• Diffusive propagation of cosmic rays from supernova remnants in the Galaxy. II: anisotropy

  2011cited by this paper
• A Cocoon of Freshly Accelerated Cosmic Rays Detected by Fermi in the Cygnus Superbubble

  2011cited by this paper
• Discovery of extended VHE γ-ray emission from the vicinity of the young massive stellar cluster Westerlund 1

  2011cited by this paper
• Cosmic-Ray Propagation: Nonlinear Diffusion Parallel and Perpendicular to Mean Magnetic Field

  2007cited by this paper
• The abundance discrepancy – recombination line versus forbidden line abundances for a northern sample of galactic planetary nebulae

  2005cited by this paper
• Cosmic-Ray Scattering and Streaming in Compressible Magnetohydrodynamic Turbulence

  2004cited by this paper
• The Milky Way in Molecular Clouds: A New Complete CO Survey

  2000cited by this paper
• Toward a theory of interstellar turbulence. 2. Strong Alfvenic turbulence

  1994cited by this paper
• Particle acceleration at astrophysical shocks: A theory of cosmic ray origin

  1987cited by this paper
• Photoelectric heating of interstellar gas

  1978cited by this paper
• The Effect of Wave-Particle Interactions on the Propagation of Cosmic Rays

  1969cited by this paper
• Cosmic Rays from Super-Novae

  1934cited by this paper

• No citing papers are available for this paper.