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Nuclear Physics News, ISSN 1061-9127, 07/2019, Volume 29, Issue 3, pp. 22 - 27
The positron, the antiparticle of the electron, was discovered in 1932 by David Anderson when a shower of cosmic rays hit his cloud chamber [1]. Positrons are... 
Cosmic ray showers | Particle accelerators | Thunderstorms | Beta rays | Beta decay | Lightning | Positrons | Elementary particles | Atmospheric physics | Positron annihilation | Cloud chambers | Cosmic rays
Journal Article
Journal of The Surface Finishing Society of Japan, ISSN 0915-1869, 06/2018, Volume 69, Issue 6, pp. 230 - 233
Journal Article
Hyomen Gijutsu = Journal of the Surface Finishing Society of Japan, ISSN 0915-1869, 01/2018, Volume 69, Issue 6, p. 230
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 03/2019, Volume 483, Issue 3, pp. 4175 - 4186
There is growing evidence that a clear distinction between magnetars and radio pulsars may not exist, implying the population of neutron stars that exhibit... 
SOFT GAMMA-REPEATERS | RADIATIVE MECHANISM | SGR 1900+14 | radio continuum: transients | stars: magnetars | pulsars: general | NEUTRON-STARS | 1E 1547.0-5408 | MAGNETOSPHERES | MODEL | GIANT FLARE | stars: neutron | ASTRONOMY & ASTROPHYSICS | X-RAY | EMISSION | pulsars: individual: PSR J1119-6127 | X-rays: bursts | Physics - High Energy Astrophysical Phenomena
Journal Article
by Aharonian, Felix and Akamatsu, Hiroki and Akimoto, Fumie and Allen, Steven W and Anabuki, Naohisa and Angelini, Lorella and Arnaud, Keith and Audard, Marc and Awaki, Hisamitsu and Axelsson, Magnus and Bamba, Aya and Bautz, Marshall and Blandford, Roger and Brenneman, Laura and Brown, Gregory V and Bulbul, Esra and Cackett, Edward and Chernyakova, Maria and Chiao, Meng and Coppi, Paolo and Costantini, Elisa and De Plaa, Jelle and Den Herder, Jan-Willem and Done, Chris and Dotani, Tadayasu and Ebisawa, Ken and Eckart, Megan and Enoto, Teruaki and Ezoe, Yuichiro and Fabian, Andrew C and Ferrigno, Carlo and Foster, Adam and Fujimoto, Ryuichi and Fukazawa, Yasushi and Furuzawa, Akihiro and Galeazzi, Massimiliano and Gallo, Luigi and Gandhi, Poshak and Giustini, Margherita and Goldwurm, Andrea and Gu, Liyi and Guainazzi, Matteo and Haba, Yoshito and Hagino, Kouichi and Hamaguchi, Kenji and Harrus, Ilana and Hatsukade, Isamu and Hayashi, Katsuhiro and Hayashi, Takayuki and Hayashida, Kiyoshi and Hiraga, Junko and Hornschemeier, Ann and Hoshino, Akio and Hughes, John and Iizuka, Ryo and Inoue, Hajime and Inoue, Yoshiyuki and Ishibashi, Kazunori and Ishida, Manabu and Ishikawa, Kumi and Ishisaki, Yoshitaka and Itoh, Masayuki and Iyomoto, Naoko and Kaastra, Jelle and Kallman, Timothy and Kamae, Tuneyoshi and Kara, Erin and Kataoka, Jun and Katsuda, Satoru and Katsuta, Junichiro and Kawaharada, Madoka and Kawai, Nobuyuki and Kelley, Richard and Khangulyan, Dmitry and Kilbourne, Caroline and King, Ashley and Kitaguchi, Takao and Kitamoto, Shunji and Kitayama, Tetsu and Kohmura, Takayoshi and Kokubun, Motohide and Koyama, Shu and Koyama, Katsuji and Kretschmar, Peter and Krimm, Hans and Kubota, Aya and Kunieda, Hideyo and Laurent, Philippe and Lebrun, François and Lee, Shiu-Hang and Leutenegger, Maurice and Limousin, Olivier and Loewenstein, Michael and Long, Knox S and Lumb, David and Madejski, Grzegorz and Maeda, Yoshitomo and Maier, Daniel and Makishima, Kazuo and Markevitch, Maxim and ... and Hitomi Collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States)
Nature, ISSN 0028-0836, 07/2016, Volume 535, Issue 7610, pp. 117 - 121
Clusters of galaxies are the most massive gravitationally bound objects in the Universe and are still forming. They are thus important probes(1) of... 
NGC 1275 | GALAXY CLUSTERS | TURBULENT VELOCITY | MULTIDISCIPLINARY SCIENCES | LINE | GAS | NGC-1275 | CONSTRAINTS | X-RAY SPECTROSCOPY | XMM-NEWTON | FEEDBACK | Clusters | Observations | Stars | Cosmology | Astrophysics | Velocity | Stars & galaxies | ASTRONOMY AND ASTROPHYSICS | GRQC | ASTRO
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2014, Volume 443, Issue 4, p. 3586
  The ultrastrong magnetic field of magnetars modifies the neutrino cross-section due to the parity violation of the weak interaction and can induce asymmetric... 
Cooling | Anisotropy | Neutrinos | Radiation | Effects | Magnetic fields | Astronomy
Journal Article
Reports on Progress in Physics, ISSN 0034-4885, 10/2019, Volume 82, Issue 10, p. 106901
Journal Article
PHYSICAL REVIEW LETTERS, ISSN 0031-9007, 08/2019, Volume 123, Issue 6, p. 061103
During a winter thunderstorm on 24 November 2017, a strong burst of gamma rays with energies up to similar to 10 MeV was detected coincident with a lightning... 
PHYSICS, MULTIDISCIPLINARY | GROUND-LEVEL | Gamma rays | Bursting strength | Thunderstorms | Computer simulation | Detectors | Nuclear power plants | Electron avalanche | Scintillation | Sea level | Ionization chambers
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 443, Issue 4, pp. 3586 - 3593
The ultrastrong magnetic field of magnetars modifies the neutrino cross-section due to the parity violation of the weak interaction and can induce asymmetric... 
Pulsars: general | Radiative transfer | Magnetic fields | Neutrinos | Stars: magnetars | magnetic fields | stars: magnetars | REPEATERS | neutrinos | X-RAY PULSARS | DECAY | radiative transfer | pulsars: general | EVOLUTION | ASTRONOMY & ASTROPHYSICS | CHANDRA | CORE-COLLAPSE SUPERNOVAE | STARS | SPECTRUM
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 01/2019, Volume 71, Issue 1
Abstract Archival NuSTAR data of the magnetar 4U 0142+61, acquired in 2014 March for a total time span of 258 ks, were analyzed. This is to reconfirm the 55 ks... 
FIELDS | stars: magnetars | REPEATERS | stars: magnetic fields | ASTRONOMY & ASTROPHYSICS | stars: individual (4U 0142+61) | DETECTOR | NEUTRON-STARS | SOFT | stars: neutron | BROAD-BAND | Physics - High Energy Astrophysical Phenomena
Journal Article
Nature, ISSN 0028-0836, 01/2016, Volume 529, Issue 7584, pp. 54 - 58
How black holes accrete surrounding matter is a fundamental yet unsolved question in astrophysics. It is generally believed that matter is absorbed into black... 
PARALLAX DISTANCE | TRANSIENT GS 2023+338 | RELATIVISTIC JETS | V4641 SAGITTARII | GRS 1915+105 | IGR J17091-3624 | MULTIDISCIPLINARY SCIENCES | LIGHT CURVES | COMPACT JET | OUTBURST | X-RAY BINARY | Usage | Spectrometer | Fluctuations (Physics) | Analysis | Telescopes | Astrophysics | Black holes | Accretion disks | Light | Physics - High Energy Astrophysical Phenomena
Journal Article