Sökning: WFRF:(Inoue Akio K.) > Hitomi X-ray observ...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 10456naa a2202689 4500 | |
001 | oai:DiVA.org:su-158932 | |
003 | SwePub | |
008 | 180821s2018 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1589322 URI |
024 | 7 | a https://doi.org/10.1093/pasj/psy0272 DOI |
040 | a (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Aharonian, Felix4 aut |
245 | 1 0 | a Hitomi X-ray observation of the pulsar wind nebula G21.5-0.9 |
264 | c 2018-04-03 | |
264 | 1 | b Oxford University Press (OUP),c 2018 |
338 | a print2 rdacarrier | |
520 | a We present results from the Hitomi X-ray observation of a young composite-type supernova remnant (SNR) G21.5-0.9, whose emission is dominated by the pulsar wind nebula (PWN) contribution. The X-ray spectra in the 0.8-80 keV range obtained with the Soft X-ray Spectrometer (SXS), Soft X-ray Imager, and Hard X-ray Imager (HXI) show a significant break in the continuum as previously found with the NuSTAR observation. After taking into account all known emissions from the SNR other than the PWN itself, we find that the Hitomi spectra can be fitted with a broken power law with photon indices of Gamma(1) = 1.74 +/- 0.02 and Gamma(2) = 2.14 +/- 0.01 below and above the break at 7.1 +/- 0.3 keV, which is significantly lower than the NuSTAR result (similar to 9.0 keV). The spectral break cannot be reproduced by time-dependent particle injection one-zone spectral energy distribution models, which strongly indicates that a more complex emission model is needed, as suggested by recent theoretical models. We also search for narrow emission or absorption lines with the SXS, and perform a timing analysis of PSR J1833-1034 with the HXI and the Soft Gamma-ray Detector. No significant pulsation is found from the pulsar. However, unexpectedly, narrow absorption line features are detected in the SXS data at 4.2345 keV and 9.296 keV with a significance of 3.65 sigma. While the origin of these features is not understood, their mere detection opens up a new field of research and was only possible with the high resolution, sensitivity, and ability to measure extended sources provided by an X-ray microcalorimeter. | |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a ISM: individual objects (G21.5-0.9) | |
653 | a ISM: supernova remnants | |
653 | a pulsars: individual (PSR J1833-1034) | |
700 | 1 | a Akamatsu, Hiroki4 aut |
700 | 1 | a Akimoto, Fumie4 aut |
700 | 1 | a Allen, Steven W.4 aut |
700 | 1 | a Angelini, Lorella4 aut |
700 | 1 | a Audard, Marc4 aut |
700 | 1 | a Awaki, Hisamitsu4 aut |
700 | 1 | a Axelsson, Magnusu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)aaxe |
700 | 1 | a Bamba, Aya4 aut |
700 | 1 | a Bautz, Marshall W.4 aut |
700 | 1 | a Blandford, Roger4 aut |
700 | 1 | a Brenneman, Laura W.4 aut |
700 | 1 | a Brown, Gregory4 aut |
700 | 1 | a Bulbul, Esra4 aut |
700 | 1 | a Cackett, Edward M.4 aut |
700 | 1 | a Chernyakova, Maria4 aut |
700 | 1 | a Chiao, Meng P.4 aut |
700 | 1 | a Coppi, Paolo S.4 aut |
700 | 1 | a Costantini, Elisa4 aut |
700 | 1 | a de Plaa, Jelle4 aut |
700 | 1 | a de Vries, Cor P.4 aut |
700 | 1 | a den Herder, Jan-Willem4 aut |
700 | 1 | a Done, Chris4 aut |
700 | 1 | a Dotani, Tadayasu4 aut |
700 | 1 | a Ebisawa, Ken4 aut |
700 | 1 | a Eckart, Megan E.4 aut |
700 | 1 | a Enoto, Teruaki4 aut |
700 | 1 | a Ezoe, Yuichiro4 aut |
700 | 1 | a Fabian, Andrew C.4 aut |
700 | 1 | a Ferrigno, Carlo4 aut |
700 | 1 | a Foster, Adam R.4 aut |
700 | 1 | a Fujimoto, Ryuichi4 aut |
700 | 1 | a Fukazawa, Yasushi4 aut |
700 | 1 | a Furuzawa, Akihiro4 aut |
700 | 1 | a Galeazzi, Massimiliano4 aut |
700 | 1 | a Gallo, Luigi C.4 aut |
700 | 1 | a Gandhi, Poshak4 aut |
700 | 1 | a Giustini, Margherita4 aut |
700 | 1 | a Goldwurm, Andrea4 aut |
700 | 1 | a Gu, Liyi4 aut |
700 | 1 | a Guainazzi, Matteo4 aut |
700 | 1 | a Haba, Yoshito4 aut |
700 | 1 | a Hagino, Kouichi4 aut |
700 | 1 | a Hamaguchi, Kenji4 aut |
700 | 1 | a Harrus, Ilana M.4 aut |
700 | 1 | a Hatsukade, Isamu4 aut |
700 | 1 | a Hayashi, Katsuhiro4 aut |
700 | 1 | a Hayashi, Takayuki4 aut |
700 | 1 | a Hayashida, Kiyoshi4 aut |
700 | 1 | a Hiraga, Junko S.4 aut |
700 | 1 | a Hornschemeier, Ann4 aut |
700 | 1 | a Hoshino, Akio4 aut |
700 | 1 | a Hughes, John P.4 aut |
700 | 1 | a Ichinohe, Yuto4 aut |
700 | 1 | a Iizuka, Ryo4 aut |
700 | 1 | a Inoue, Hajime4 aut |
700 | 1 | a Inoue, Yoshiyuki4 aut |
700 | 1 | a Ishida, Manabu4 aut |
700 | 1 | a Ishikawa, Kumi4 aut |
700 | 1 | a Ishisaki, Yoshitaka4 aut |
700 | 1 | a Iwai, Masachika4 aut |
700 | 1 | a Kaastra, Jelle4 aut |
700 | 1 | a Kallman, Tim4 aut |
700 | 1 | a Kamae, Tsuneyoshi4 aut |
700 | 1 | a Kataoka, Jun4 aut |
700 | 1 | a Katsuda, Satoru4 aut |
700 | 1 | a Kawai, Nobuyuki4 aut |
700 | 1 | a Kelley, Richard L.4 aut |
700 | 1 | a Kilbourne, Caroline A.4 aut |
700 | 1 | a Kitaguchi, Takao4 aut |
700 | 1 | a Kitamoto, Shunji4 aut |
700 | 1 | a Kitayama, Tetsu4 aut |
700 | 1 | a Kohmura, Takayoshi4 aut |
700 | 1 | a Kokubun, Motohide4 aut |
700 | 1 | a Koyama, Katsuji4 aut |
700 | 1 | a Koyama, Shu4 aut |
700 | 1 | a Kretschmar, Peter4 aut |
700 | 1 | a Krimm, Hans A.4 aut |
700 | 1 | a Kubota, Aya4 aut |
700 | 1 | a Kunieda, Hideyo4 aut |
700 | 1 | a Laurent, Philippe4 aut |
700 | 1 | a Lee, Shiu-Hang4 aut |
700 | 1 | a Leutenegger, Maurice A.4 aut |
700 | 1 | a Limousin, Olivier4 aut |
700 | 1 | a Loewenstein, Michael4 aut |
700 | 1 | a Long, Knox S.4 aut |
700 | 1 | a Lumb, David4 aut |
700 | 1 | a Madejski, Greg4 aut |
700 | 1 | a Maeda, Yoshitomo4 aut |
700 | 1 | a Maier, Daniel4 aut |
700 | 1 | a Makishima, Kazuo4 aut |
700 | 1 | a Markevitch, Maxim4 aut |
700 | 1 | a Matsumoto, Hironori4 aut |
700 | 1 | a Matsushita, Kyoko4 aut |
700 | 1 | a McCammon, Dan4 aut |
700 | 1 | a McNamara, Brian R.4 aut |
700 | 1 | a Mehdipour, Missagh4 aut |
700 | 1 | a Miller, Eric D.4 aut |
700 | 1 | a Miller, Jon M.4 aut |
700 | 1 | a Mineshige, Shin4 aut |
700 | 1 | a Mitsuda, Kazuhisa4 aut |
700 | 1 | a Mitsuishi, Ikuyuki4 aut |
700 | 1 | a Miyazawa, Takuya4 aut |
700 | 1 | a Mizuno, Tsunefumi4 aut |
700 | 1 | a Mori, Hideyuki4 aut |
700 | 1 | a Mori, Koji4 aut |
700 | 1 | a Mukai, Koji4 aut |
700 | 1 | a Murakami, Hiroshi4 aut |
700 | 1 | a Mushotzky, Richard F.4 aut |
700 | 1 | a Nakagawa, Takao4 aut |
700 | 1 | a Nakajima, Hiroshi4 aut |
700 | 1 | a Nakamori, Takeshi4 aut |
700 | 1 | a Nakashima, Shinya4 aut |
700 | 1 | a Nakazawa, Kazuhiro4 aut |
700 | 1 | a Nobukawa, Kumiko K.4 aut |
700 | 1 | a Nobukawa, Masayoshi4 aut |
700 | 1 | a Noda, Hirofumi4 aut |
700 | 1 | a Odaka, Hirokazu4 aut |
700 | 1 | a Ohashi, Takaya4 aut |
700 | 1 | a Ohno, Masanori4 aut |
700 | 1 | a Okajima, Takashi4 aut |
700 | 1 | a Ota, Naomi4 aut |
700 | 1 | a Ozaki, Masanobu4 aut |
700 | 1 | a Paerels, Frits4 aut |
700 | 1 | a Paltani, Stephane4 aut |
700 | 1 | a Petre, Robert4 aut |
700 | 1 | a Pinto, Ciro4 aut |
700 | 1 | a Porter, Frederick S.4 aut |
700 | 1 | a Pottschmidt, Katja4 aut |
700 | 1 | a Reynolds, Christopher S.4 aut |
700 | 1 | a Safi-Harb, Samar4 aut |
700 | 1 | a Saito, Shinya4 aut |
700 | 1 | a Sakai, Kazuhiro4 aut |
700 | 1 | a Sasaki, Toru4 aut |
700 | 1 | a Sato, Goro4 aut |
700 | 1 | a Sato, Kosuke4 aut |
700 | 1 | a Sato, Rie4 aut |
700 | 1 | a Sawada, Makoto4 aut |
700 | 1 | a Schartel, Norbert4 aut |
700 | 1 | a Serlemtsos, Peter J.4 aut |
700 | 1 | a Seta, Hiromi4 aut |
700 | 1 | a Shidatsu, Megumi4 aut |
700 | 1 | a Simionescu, Aurora4 aut |
700 | 1 | a Smith, Randall K.4 aut |
700 | 1 | a Soong, Yang4 aut |
700 | 1 | a Stawarz, Lukasz4 aut |
700 | 1 | a Sugawara, Yasuharu4 aut |
700 | 1 | a Sugita, Satoshi4 aut |
700 | 1 | a Szymkowiak, Andrew4 aut |
700 | 1 | a Tajima, Hiroyasu4 aut |
700 | 1 | a Takahashi, Hiromitsu4 aut |
700 | 1 | a Takahashi, Tadayuki4 aut |
700 | 1 | a Takeda, Shinichiro4 aut |
700 | 1 | a Takei, Yoh4 aut |
700 | 1 | a Tamagawa, Toru4 aut |
700 | 1 | a Tamura, Takayuki4 aut |
700 | 1 | a Tanaka, Takaaki4 aut |
700 | 1 | a Tanaka, Yasuo4 aut |
700 | 1 | a Tanaka, Yasuyuki T.4 aut |
700 | 1 | a Tashiro, Makoto S.4 aut |
700 | 1 | a Tawara, Yuzuru4 aut |
700 | 1 | a Terada, Yukikatsu4 aut |
700 | 1 | a Terashima, Yuichi4 aut |
700 | 1 | a Tombesi, Francesco4 aut |
700 | 1 | a Tomida, Hiroshi4 aut |
700 | 1 | a Tsuboi, Yohko4 aut |
700 | 1 | a Tsujimoto, Masahiro4 aut |
700 | 1 | a Tsunemi, Hiroshi4 aut |
700 | 1 | a Tsuru, Takeshi Go4 aut |
700 | 1 | a Uchida, Hiroyuki4 aut |
700 | 1 | a Uchiyama, Hideki4 aut |
700 | 1 | a Uchiyama, Yasunobu4 aut |
700 | 1 | a Ueda, Shutaro4 aut |
700 | 1 | a Uno, Shinichiro4 aut |
700 | 1 | a Ueda, Yoshihiro4 aut |
700 | 1 | a Urry, C. Megan4 aut |
700 | 1 | a Ursino, Eugenio4 aut |
700 | 1 | a Watanabe, Shin4 aut |
700 | 1 | a Werner, Norbert4 aut |
700 | 1 | a Wilkins, Dan R.4 aut |
700 | 1 | a Williams, Brian J.4 aut |
700 | 1 | a Yamada, Shinya4 aut |
700 | 1 | a Yamaguchi, Hiroya4 aut |
700 | 1 | a Yamaoka, Kazutaka4 aut |
700 | 1 | a Yamasaki, Noriko Y.4 aut |
700 | 1 | a Yamauchi, Makoto4 aut |
700 | 1 | a Yamauchi, Shigeo4 aut |
700 | 1 | a Yaqoob, Tahir4 aut |
700 | 1 | a Yatsu, Yoichi4 aut |
700 | 1 | a Yonetoku, Daisuke4 aut |
700 | 1 | a Zhuravleva, Irina4 aut |
700 | 1 | a Zoghbi, Abderahmen4 aut |
700 | 1 | a Sato, Toshiki4 aut |
700 | 1 | a Nakaniwa, Nozomu4 aut |
700 | 1 | a Murakami, Hiroaki4 aut |
700 | 1 | a Guest, Benson4 aut |
710 | 2 | a Stockholms universitetb Fysikum4 org |
773 | 0 | t Publications of the Astronomical Society of Japand : Oxford University Press (OUP)g 70:3q 70:3x 0004-6264x 2053-051X |
856 | 4 | u https://doi.org/10.1093/pasj/psy027y Fulltext |
856 | 4 | u https://academic.oup.com/pasj/article-pdf/70/3/38/25055029/psy027.pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-158932 |
856 | 4 8 | u https://doi.org/10.1093/pasj/psy027 |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.
Kopiera och spara länken för att återkomma till aktuell vy