Results 71 to 80 of about 2,258,607 (385)
The ARGO-YBJ legacy to next generation wide field-of-view experiments
EPJ Web of Conferences, 2017 The ARGO-YBJ experiment has been in stable data taking for more than 5 years at the YangBaJing Cosmic Ray Observatory (Tibet, P.R. China, 4300 m a.s.l., 606 g/cm2).
Di Sciascio Giuseppe
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Measuring the ionisation fraction in a jet from a massive protostar
Nature Communications, 2019 The ionisation fraction of protostellar jets is key to establish their true energetics. Here, the authors determine it in a jet from a high-mass young stellar object, using multi-wavelengths observations, confirming that the ionising mechanism giving ...
R. Fedriani +9 more
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Status and recent high light results from the LHAASO experiment [PDF]
EPJ Web of ConferencesThe Large High Altitude Air Shower Observatory (LHAASO) experiment, fully operational since July 2021, is a cutting-edge facility for detecting cosmic rays and gamma rays across a wide energy range. This paper offers an overview of the current status and
Chen Songzhan
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Turning AGN Bubbles into Radio Relics with Sloshing: Modeling CR Transport with Realistic Physics
Galaxies, 2021 Radio relics are arc-like synchrotron sources at the periphery of galaxy clusters, produced by cosmic-ray electrons in a μG magnetic field, which are believed to have been (re-)accelerated by merger shock fronts.
John ZuHone +3 more
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Cosmic Rays and Particle Physics [PDF]
Acta Physica Hungarica A) Heavy Ion Physics, 2001 13 pages, 7 figures; invited talk presented at the "Symposium on Fundamental Issues in Elementary Matter", Bad Honnef, Germany, 25-29 September 2000 (to appear in Acta Physica Hungarica)
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Publisher Correction: Measuring the ionisation fraction in a jet from a massive protostar
Nature Communications, 2019 An amendment to this paper has been published and can be accessed via a link at the top of the paper.
R. Fedriani +9 more
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Propagation of Cosmic Rays: Nuclear Physics in Cosmic-Ray Studies [PDF]
AIP Conference Proceedings, 2005 The nuclei fraction in cosmic rays (CR) far exceeds the fraction of other CR species, such as antiprotons, electrons, and positrons. Thus the majority of information obtained from CR studies is based on interpretation of isotopic abundances using CR propagation models where the nuclear data and isotopic production cross sections in p- and alpha-induced
Stepan G. Mashnik +2 more
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Solar and nuclear physics uncertainties in cosmic-ray propagation [PDF]
, 2017 Recent data released by the AMS experiment on the primary spectra and secondary-to-primary ratios in cosmic rays (CRs) can pose tight constraints to astrophysical models of CR acceleration and transport in the Galaxy, thereby providing a robust baseline ...
N. Tomassetti
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Physics of Cosmic Masers [PDF]
Symposium - International Astronomical Union, 1988 Natural masers, which emit powerful narrow-band radiation in molecular microwave lines, were discovered about 20 years ago. They draw the astrophysicist's attention in two ways: 1) as a unique physical phenomenon and 2) as very informative probes of physical conditions in those astrophysical objects (very young and very old stars) with which they are ...
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