Zobrazeno 1 - 10
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pro vyhledávání: '"P Mertsch"'
Supernova remnants (SNRs) have long been suspected to be the primary sources of Galactic cosmic rays. Over the past decades, great strides have been made in the modelling of particle acceleration, magnetic field amplification, and escape from SNRs. Y
Externí odkaz:
http://arxiv.org/abs/2409.11012
Autor:
Söding, Laurin, Edenhofer, Gordian, Enßlin, Torsten A., Frank, Philipp, Kissmann, Ralf, Phan, Vo Hong Minh, Ramírez, Andrés, Zhandinejad, Hanieh, Mertsch, Philipp
The spatial distribution of the gaseous components of the Milky Way is of great importance for a number of different fields, e.g. Galactic structure, star formation and cosmic rays. However, obtaining distance information to gaseous clouds in the int
Externí odkaz:
http://arxiv.org/abs/2407.02859
Autor:
Ramírez, Andrés, Edenhofer, Gordian, Enßlin, Torsten A., Frank, Philipp, Mertsch, Philipp, Phan, Vo Hong Minh, Söding, Laurin, Zhandinejad, Hanieh, Kissmann, Ralf
Cosmic rays (CRs) play a major role in the dynamics of the interstellar medium (ISM). Their interactions and transport ionize, heat, and push the ISM thereby coupling different regions of it. The spatial distribution of CRs depends on the distributio
Externí odkaz:
http://arxiv.org/abs/2407.02410
Cosmic rays are the only agent capable of ionizing the interior of dense molecular clouds and, thus, they are believed to play an essential role in determining the physical and chemical evolution of star-forming regions. In this work, we aim to study
Externí odkaz:
http://arxiv.org/abs/2402.05915
Autor:
Giuffrida, R., Miceli, M., Ravikularaman, S., Phan, V. H. M., Gabici, S., Mertsch, P., Orlando, S., Bocchino, F.
Supernova remnants interacting with molecular/atomic clouds are interesting X-ray sources to study broadband nonthermal emission. X-ray line emission in these systems can be produced by different processes, e.g. low energy cosmic rays interacting wit
Externí odkaz:
http://arxiv.org/abs/2401.05001
Publikováno v:
PoS(ICRC2023)658
Due to our vantage point in the disk of the Galaxy, its 3D structure is not directly accessible. However, knowing the spatial distribution, e.g. of atomic and molecular hydrogen gas is of great importance for interpreting and modelling cosmic ray dat
Externí odkaz:
http://arxiv.org/abs/2309.14075
Publikováno v:
PoS ICRC2023 (2023) 687
Cosmic rays of energies up to a few PeV are believed to be of galactic origin, yet individual sources have still not been firmly identified. Due to inelastic collisions with the interstellar gas, cosmic-ray nuclei produce a diffuse flux of high-energ
Externí odkaz:
http://arxiv.org/abs/2309.02860
Autor:
Maurin, D., Ahlers, M., Dembinski, H., Haungs, A., Mangeard, P. -S., Melot, F., Mertsch, P., Wochele, D., Wochele, J.
Publikováno v:
EPJC 83, 971 (2023)
The cosmic-ray database, CRDB, has been gathering cosmic-ray data for the community since 2013. We present a new release, CRDB v4.1, providing many new quantities and data sets, with several improvements made on the code and web interface, and with n
Externí odkaz:
http://arxiv.org/abs/2306.08901
Observations of the vicinity of a variety of galactic gamma-ray sources have indicated a local suppression of diffusivity of cosmic rays by up to three orders of magnitude. However, the impact of these low-diffusion zones on \emph{global} properties
Externí odkaz:
http://arxiv.org/abs/2305.10337
Autor:
Mümmler C, Mertsch P, Barnikel M, Haubner F, Schönermarck U, Grabmaier U, Schulze-Koops H, Behr J, Kneidinger N, Milger K
Publikováno v:
Journal of Asthma and Allergy, Vol Volume 17, Pp 557-572 (2024)
Carlo Mümmler,1 Pontus Mertsch,1 Michaela Barnikel,1 Frank Haubner,2 Ulf Schönermarck,3 Ulrich Grabmaier,4 Hendrik Schulze-Koops,5 Jürgen Behr,1 Nikolaus Kneidinger,1,6 Katrin Milger1 1Department of Medicine V, LMU University Hospital, LMU Munich,
Externí odkaz:
https://doaj.org/article/4876db04923144e59915c062279f0c76
