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by Aharonian, F and Akhperjanian, A. G and Anton, G and Barres de Almeida, U and Bazer-Bachi, A. R and Becherini, Y and Behera, B and Bernlöhr, K and Boisson, C and Bochow, A and Borrel, V and Brion, E and Brucker, J and Brun, P and Bühler, R and Bulik, T and Büsching, I and Boutelier, T and Chadwick, P. M and Charbonnier, A and Chaves, R. C. G and Cheesebrough, A and Chounet, L.-M and Clapson, A. C and Coignet, G and Dalton, M and Daniel, M. K and Davids, I. D and Degrange, B and Deil, C and Dickinson, H. J and Djannati-Ataï, A and Domainko, W and O'C. Drury, L and Dubois, F and Dubus, G and Dyks, J and Dyrda, M and Egberts, K and Emmanoulopoulos, D and Espigat, P and Farnier, C and Feinstein, F and Fiasson, A and Förster, A and Fontaine, G and Füßling, M and Gabici, S and Gallant, Y. A and Gérard, L and Giebels, B and Glicenstein, J. F and Glück, B and Goret, P and Göhring, D and Hauser, D and Hauser, M and Heinz, S and Heinzelmann, G and Henri, G and Hermann, G and Hinton, J. A and Hoffmann, A and Hofmann, W and Holleran, M and Hoppe, S and Horns, D and Jacholkowska, A and de Jager, O. C and Jahn, C and Jung, I and Katarzyński, K and Katz, U and Kaufmann, S and Kendziorra, E and Kerschhaggl, M and Khangulyan, D and Khélifi, B and Keogh, D and Kluźniak, W and Komin, Nu and Kosack, K and Lamanna, G and Lenain, J.-P and Lohse, T and Marandon, V and Martin, J. M and Martineau-Huynh, O and Marcowith, A and Maurin, D and McComb, T. J. L and Medina, M. C and Moderski, R and Moulin, E and Naumann-Godo, M and de Naurois, M and Nedbal, D and Nekrassov, D and Niemiec, J and Nolan, S. J and ...
The Astrophysical Journal, ISSN 0004-637X, 05/2009, Volume 696, Issue 2, pp. L150 - L155
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 04/2016, Volume 588, p. A73
The propagation of cosmic rays or energetic charged particles in magnetized turbulence is a complex problem which involves non-linear wave-particle... 
Magnetohydrodynamics (MHD) | Turbulence | Cosmic rays | Methods: numerical | Cosmic ray propagation | Turbulent flow | Computational fluid dynamics | Magnetohydrodynamic turbulence | Modules | Fluid flow | Mathematical models | Physics - High Energy Astrophysical Phenomena | Physics | Astrophysics | High Energy Astrophysical Phenomena
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 06/2010, Volume 515, Issue 11, p. A90
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2009, Volume 393, Issue 2, pp. 587 - 597
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622
Context. Cosmic rays propagate through the galactic scales down to the smaller scales at which stars form. Cosmic rays are close to energy equipartition with... 
Cosmic ray propagation | Turbulence | Turbulent flow | Parameters | Computer simulation | Propagation | Computational fluid dynamics | Cosmic rays | Pressure gradients | Flow stability | Gamma rays | Thermal instability | Trapping | Flux density | Energy | Gas flow | Evolution | Scaling | Instability | Interstellar medium | Diffusion | Diffusion coefficient | Interstellar gas | Interstellar matter
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2015, Volume 582, pp. L13 - 4
The main signature of the interaction between cosmic rays and molecular clouds is the high ionisation degree. This decreases towards the densest parts of a... 
Stars: protostars | ISM: jets and outflows | Cosmic rays | DG TAURI | stars: protostars | PARTICLES | SLITLESS | COLLIMATION | cosmic rays | DIFFUSIVE SHOCK ACCELERATION | ASTRONOMY & ASTROPHYSICS | JET | STELLAR | EMISSION | IONIZATION | SUB-ARCSECOND | Collapse | Clouds | Star formation | Particle acceleration | Signatures | Acceleration | Energetic particles | Protostars | Physics | Astrophysics
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 09/2019, Volume 630, p. A72
Context. Radio observations at metre-centimetre wavelengths shed light on the nature of the emission of H II regions. Usually this category of objects is... 
ENERGY | acceleration of particles | radio continuum: ISM | STAR-FORMATION | MORPHOLOGIES | REMNANT | stars: formation | PARTICLE-ACCELERATION | H II regions | cosmic rays | DIFFUSIVE SHOCK ACCELERATION | ASTRONOMY & ASTROPHYSICS | RADIO | MAGNETIC-FIELD | SYNCHROTRON EMISSION
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2019, Volume 490, Issue 1, pp. 1156 - 1165
ABSTRACT We use particle-in-magnetohydrodynamics-cells to model particle acceleration and magnetic field amplification in a high-Mach, parallel shock in three... 
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 10/2019
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2018, Volume 479, Issue 4, pp. 4470 - 4485
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2016, Volume 461, Issue 4, pp. 3552 - 3562
Supernova remnants are believed to be the main sources of galactic cosmic rays (CR). Within this framework, particles are accelerated at supernova remnant... 
Cosmic rays | MAGNETOHYDRODYNAMIC TURBULENCE | SHOCK ACCELERATION | PARTICLE-ACCELERATION | cosmic rays | MOLECULAR CLOUDS | ASTRONOMY & ASTROPHYSICS | SUPERBUBBLES | GAMMA-RAYS | ENERGETIC PARTICLES | EMISSION | PROPAGATION | GALAXY | Physics - High Energy Astrophysical Phenomena
Journal Article