Probing the relation between progenitors and maximum brightness for Type Ia supernovae through X-ray and optical observations of supernova remnants

通过超新星遗迹的 X 射线和光学观测探讨 Ia 型超新星前身与最大亮度之间的关系

• 批准号: 16K17673
• 负责人: Katsuda Satoru
• 金额: $ 2.58万
• 依托单位: Saitama University (2017-2018)Chuo University (2016)
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for Young Scientists (B)
• 财政年份: 2016
• 资助国家: 日本
• 起止时间: 2016-04-01 至 2019-03-31
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/en/grant/KAKENHI-PROJECT-16K17673/
• 关键词: 超新星残骸; Ｘ線観測; 可視光観測; Ｘ線γ線天文学

项目成果

Measurement of the X-ray proper motion in the south-east rim of RX J1713.7-3946

RX J1713.7-3946东南缘X射线自行测量

• DOI: 10.1051/0004-6361/201629618
• 发表时间: 2017
• 期刊: Astronomy & Astrophysics
• 影响因子: 6.5
• 作者: Acero;Fabio; Katsuda;Satoru; Ballet;Jean; Petre;Robert
• 通讯作者: Robert

Measuring Cosmic-Ray Acceleration Efficiencies in Supernova Remnants

测量超新星遗迹中的宇宙射线加速效率

• 发表时间: 2017
• 作者: Yasuharu Sugawara;Yoshitomo Maeda;Yohko Tsuboi;Satoru Katsuda
• 通讯作者: Satoru Katsuda

「KWFC」Hα測光観測による超新星残骸G156.2+5.7の膨張率測定

“KWFC”利用Hα光度观测测量超新星遗迹G156.2+5.7的膨胀率

• 发表时间: 2016
• 作者: 勝田 哲、田中雅臣、諸隈智貴、Robert Fesen;& Dan Milisavljevic
• 通讯作者: & Dan Milisavljevic

Hitomi X-ray observation of the pulsar wind nebula G21.5-0.9

瞳X射线观测脉冲星风星云G21.5-0.9

• DOI: 10.1093/pasj/psy027
• 发表时间: 2018
• 期刊: Publications of the Astronomical Society of Japan
• 影响因子: 2.3
• 作者: Hitomi Collaboration;Aharonian Felix;...;Kohmura Takayoshi...;et al (他191名）
• 通讯作者: et al (他191名）

Solar abundance ratios of the iron-peak elements in the Perseus cluster

• DOI: 10.1038/nature24301
• 发表时间: 2017-11
• 期刊: Nature
• 影响因子: 64.8
• 作者: Felix Hiroki Fumie Steven W. Lorella Marc Hisamitsu Magn Aharonian Akamatsu Akimoto Allen Angelini Audard A-Felix-Hiroki-Fumie-Steven-W.-Lorella-Marc-Hisamitsu;F. Aharonian;H. Akamatsu;F. Akimoto;S. Allen;L. Angelini;M. Audard;H. Awaki;M. Axelsson;A. Bamba;M. Bautz;R. Blandford;L. Brenneman;G. V. Brown;E. Bulbul;E. Cackett;M. Chernyakova;M. Chiao;P. Coppi;E. Costantini;J. de Plaa;J. D. den Herder;C. Done;T. Dotani;K. Ebisawa;M. Eckart;T. Enoto;Y. Ezoe;A. Fabian;C. Ferrigno;A. Foster;R. Fujimoto;Y. Fukazawa;A. Furuzawa;M. Galeazzi;L. Gallo;P. Gandhi;M. Giustini;A. Goldwurm;L. Gu;M. Guainazzi;Y. Haba;K. Hagino;K. Hamaguchi;I. Harrus;I. Hatsukade;K. Hayashi;T. Hayashi;K. Hayashida;J. Hiraga;A. Hornschemeier;A. Hoshino;J. Hughes;Y. Ichinohe;R. Iizuka;H. Inoue;Y. Inoue;M. Ishida;K. Ishikawa;Y. Ishisaki;M. Iwai;J. Kaastra;T. Kallman;T. Kamae;J. Kataoka;S. Katsuda;N. Kawai;R. Kelley;C. Kilbourne;T. Kitaguchi;S. Kitamoto;T. Kitayama;T. Kohmura;M. Kokubun;K. Koyama;S. Koyama;P. Kretschmar;H. Krimm;A. Kubota;H. Kunieda;P. Laurent;Shiu-Hang Lee;M. Leutenegger;Olivier Limousine;M. Loewenstein;K. Long;D. Lumb;G. Madejski;Y. Maeda;D. Maier;K. Makishima;M. Markevitch;H. Matsumoto;K. Matsushita;D. McCammon;B. McNamara;M. Mehdipour;E. Miller;Jonathan M. Miller;S. Mineshige;K. Mitsuda;I. Mitsuishi;T. Miyazawa;T. Mizuno;H. Mori;K. Mori;K. Mukai;H. Murakami;R. Mushotzky;T. Nakagawa;H. Nakajima;T. Nakamori;S. Nakashima;K. Nakazawa;K. Nobukawa;M. Nobukawa;H. Noda;H. Odaka;T. Ohashi;M. Ohno;T. Okajima;N. Ota;M. Ozaki;F. Paerels;S. Paltani;R. Petre;C. Pinto;F. Porter;K. Pottschmidt;C. Reynolds;S. Safi-Harb;S. Saito;K. Sakai;Toru Sasaki;G. Sato;Kosuke Sato;R. Sato;M. Sawada;N. Schartel;P. Serlemitsos;H. Seta;M. Shidatsu;A. Simionescu;Randall K. Smith;Y. Soong;L. Stawarz;Y. Sugawara;S. Sugita;A. Szymkowiak;H. Tajima;Hiromitsu Takahashi;Tadayuki Takahashi;S. Takeda;Y. Takei;T. Tamagawa;T. Tamura;Takaaki Tanaka;Yasuo Tanaka;Yasuyuki T. Tanaka;M. Tashiro;Y. Tawara;Y. Terada;Y. Terashima;F. Tombesi;H. Tomida;Y. Tsuboi;M. Tsujimoto;H. Tsunemi;Takeshi Go Tsuru;H. Uchida;H. Uchiyama;Y. Uchiyama;S. Ueda;Y. Ueda;S. Uno;C. M. Urry;E. Ursino;C. D. de Vries;S. Watanabe;N. Werner;D. Wik;D. Wilkins;B. Williams;S. Yamada;H. Yamaguchi;K. Yamaoka;N. Yamasaki;M. Yamauchi;S. Yamauchi;T. Yaqoob;Y. Yatsu;D. Yonetoku;I. Zhuravleva;A. Zoghbi