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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
Astronomy and Astrophysics, ISSN 0004-6361, 01/2017, Volume 597, p. A106
A&A 597, A106 (2017) We report on the first proper motion measurement in the supernova remnant RX J1713.7-3946 using the XMM-Newton X-ray telescope on a 13... 
X-rays: ISM | ISM: supernova remnants | ISM: individual objects: RX J1713.7-3946 | Physics - High Energy Astrophysical Phenomena
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 01/2017, Volume 835, Issue 1, p. 34
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2016, Volume 826, Issue 2, pp. 108 - 108
We present deep H[alpha] images of portions of the X-ray bright, but optically faint, Galactic supernova remnant G156.2+5.7, revealing numerous and delicately... 
Supernova remnants | X rays | Filaments | Images | Spectra | Estimates | Age | Constraining
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 06/2016, Volume 824, Issue 1, p. 64
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 01/2017, Volume 597
We report on the first proper motion measurement in the supernova remnant RXJ1713.7-3946 using the XMM-Newton X-ray telescope on a 13 yr time interval. This... 
ACCELERATION | GAMMA-RAY | ISM: supernova remnants | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | GAS | REMNANT RX J1713.7-3946 | EMISSION | ISM: individual objects: RXJ1713.7-3946 | X-rays: ISM | Supernova remnants | Ejecta | X rays | Filaments | Progenitors (astrophysics) | XMM (spacecraft) | Current density | Age
Journal Article
Proceedings of Science, 2015, Volume 2015-
Conference Proceeding
Astrophysical Journal, ISSN 0004-637X, 02/2010, Volume 709, Issue 2, pp. 1387 - 1395
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2018, Volume 863, Issue 2, p. 127
We investigate a progenitor mass distribution of core-collapse supernova remnants (CCSNRs) in our Galaxy and Large and Small Magellanic Clouds for the first... 
stars: massive | ISM: supernova remnants | X-rays: general | supernovae: general | METAL ABUNDANCES | LUMINOSITY FUNCTION | ASTRONOMY & ASTROPHYSICS | RED SUPERGIANT | CHANDRA | X-RAY | 3-DIMENSIONAL SIMULATIONS | XMM-NEWTON OBSERVATIONS | STARS | MAGNESIUM-RICH EJECTA | AGE | Physics - High Energy Astrophysical Phenomena
Journal Article
European Journal of Nutrition, ISSN 1436-6207, 4/2017, Volume 56, Issue 3, pp. 949 - 964
Journal Article
AIP Conference Proceedings, ISSN 0094-243X, 01/2017, Volume 1792, Issue 1
Galactic cosmic rays are widely thought to be accelerated at supernova remnants (SNRs). SNR RX J1713.7−3946 is the strong sources of nonthermal radiation,... 
Supernova remnants | Particle accelerators | Ejecta | Galactic cosmic rays | Milky Way Galaxy | Space telescopes | X ray spectra | Nonthermal radiation | Cosmic rays | Ejection
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2018, Volume 473, Issue 1, pp. 1394 - 1406
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2016, Volume 826, Issue 2, p. 108
We present deep H alpha images of portions of the X-ray bright, but optically faint, Galactic supernova remnant G156.2+5.7, revealing numerous and delicately... 
ISM: supernova remnants | ISM: individual objects (G156.2+5.7) | shock waves | SNR G156.2+5.7 | CLOUD | NORTHEAST LIMB | DISCOVERY | PROPER MOTIONS | FILAMENTS | ASTRONOMY & ASTROPHYSICS | X-RAY-EMISSION | PRIMARY SHOCK FRONT | CYGNUS LOOP | RCW 86 | Physics - High Energy Astrophysical Phenomena
Journal Article
Astrophysical Journal, ISSN 0004-637X, 01/2018, Volume 853, Issue 1, p. 46
We present new evidence that the bright nonthermal X-ray emission features in the interior of the Cassiopeia A supernova remnant are caused by inward-moving... 
supernovae: individual (Cassiopeia A) | ISM: supernova remnants | X-rays: ISM | acceleration of particles | EJECTA | A SUPERNOVA REMNANT | 3-DIMENSIONAL STRUCTURE | SPECTROSCOPY | MAXIMUM ENERGY | REVERSE SHOCKS | ASTRONOMY & ASTROPHYSICS | CHANDRA | MAGNETIC-FIELD | SYNCHROTRON EMISSION | COSMIC-RAYS | Physics - High Energy Astrophysical Phenomena
Journal Article
Bioscience, Biotechnology, and Biochemistry, ISSN 0916-8451, 05/2014, Volume 78, Issue 5, pp. 851 - 860
Journal Article