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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 2, pp. 1778 - 1784
  We use frequency-resolved spectroscopy to examine the energy spectra of the prominent low-frequency quasi-periodic oscillation (QPO) and its harmonic in GX... 
X-rays: Individual: GX 339-4 | X-rays: Binaries | Accretion, accretion discs | Accretion disks | Star & galaxy formation | Scattering | Astronomy | Harmonics | Spectroscopy | Tracking | Inclination angle | Disks | Mathematical models | Reflection | Spectra | Physics - High Energy Astrophysical Phenomena
Journal Article
Journal of neuroinflammation, ISSN 1742-2094, 01/2019, Volume 16, Issue 1, pp. 16 - 16
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 2, pp. 1967 - 1980
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2018, Volume 480, Issue 1, pp. 752 - 759
The spectra of black hole binaries in the low/hard state are complex, with evidence formultiple different Comptonization regions contributing to the hard... 
Accretion | X-rays: binaries | Accretion discs | X-rays: individual: Cygnus X-1 | POWER SPECTRA | SOFT STATE | GX 339-4 | FAST VARIABILITY | FREQUENCY-RESOLVED SPECTROSCOPY | accretion, accretion discs | LOW/HARD STATE | REFLECTION | X-RAY BINARIES | ASTRONOMY & ASTROPHYSICS | ACCRETION | GEOMETRY | Fysik | accretion | Physical Sciences | Naturvetenskap | accretion discs | Natural Sciences
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 456, Issue 4, pp. 4354 - 4354
  At high luminosities black hole binaries show spectra with a strong disc component accompanied by an equally strong tail where at least some of the electrons... 
Luminosity | Simulation | Heating | Black holes | Astronomy | Electrons | Slopes | Binary stars | Flux | Emission | Lorentz factor | Disks | Spectra
Journal Article
Annals of Neurology, ISSN 0364-5134, 01/2011, Volume 69, Issue 1, pp. 83 - 89
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