An Hard X-ray Study of Star Formation Process
An Hard X-ray Study of Star Formation Process
恒星形成过程的硬 X 射线研究
批准号：
20540237
负责人：
TSUBOI Yohko
金额：
$2.83万
依托单位：
依托单位国家：
日本
项目类别：
Grant-in-Aid for Scientific Research (C)
财政年份：
2008
资助国家：
日本
项目状态：
已结题
起止时间：
2008 至 2010
中文摘要
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英文摘要
We detected hard X-ray emissions from protostars which are embedded in deep inside of molecular cores, and obtained physical properties (X-ray luminosities, time variabilities, plasma temperatures, etc.). We confirmed youth of the sources using infrared band data obtained with Spitzer satellite. In order to compare with X-ray properties, we also observed stellar sources with different phases and masses, and studied X-ray emitting mechanisms and acceleration of stellar winds. We further studied flare activities (flare frequencies, plasma temperatures, etc.) with extremely large X-ray luminosities, using the all-sky monitor "MAXI". We developed optics which has sensitivity for X-ray polarization.
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DOI：
10.1117/12.857875
发表时间：
2009-03
期刊：
影响因子：
--
作者：
[Tadayuki Takahashi;K. Mitsuda;R. Kelley;F. Aharonian;F. Akimoto;S. Allen;N. Anabuki;L. Angelini;K. Arnaud;H. Awaki;A. Bamba;N. Bando;M. Bautz;R. Blandford;K. Boyce;G. Brown;M. Chernyakova;P. Coppi;E. Costantini;J. Cottam;J. Crow;J. Plaa;C. D. Vries;J. Herder;M. Dipirro;C. Done;T. Dotani;K. Ebisawa;T. Enoto;Y. Ezoe;A. Fabian;R. Fujimoto;Y. Fukazawa;S. Funk;A. Furuzawa;M. Galeazzi;P. Gandhi;K. Gendreau;K. Gilmore;Y. Haba;K. Hamaguchi;I. Hatsukade;K. Hayashida;J. Hiraga;K. Hirose;A. Hornschemeier;J. Hughes;U. Hwang;R. Iizuka;K. Ishibashi;M. Ishida;K. Ishimura;Y. Ishisaki;N. Isobe;Masayuki Ito;N. Iwata;J. Kaastra;T. Kallman;T. Kamae;H. Katagiri;J. Kataoka;S. Katsuda;M. Kawaharada;N. Kawai;S. Kawasaki;Dmitry Khangaluyan;C. Kilbourne;K. Kinugasa;S. Kitamoto;T. Kitayama;T. Kohmura;M. Kokubun;T. Kosaka;T. Kotani;K. Koyama;A. Kubota;H. Kunieda;P. Laurent;F. Lebrun;O. Limousin;M. Loewenstein;K. Long;G. Madejski;Y. Maeda;K. Makishima;M. Markevitch;H. Matsumoto;K. Matsushita;D. McCammon;Jonathan M. Miller;S. Mineshige;K. Minesugi;T. Miyazawa;T. Mizuno;K. Mori;H. Mori;K. Mukai;H. Murakami;T. Murakami;R. Mushotzky;Y. Nakagawa;T. Nakagawa;H. Nakajima;T. Nakamori;K. Nakazawa;Y. Namba;M. Nomachi;S. O. Dell;H. Ogawa;M. Ogawa;K. Ogi;T. Ohashi;M. Ohno;M. Ohta;T. Okajima;N. Ota;M. Ozaki;F. Paerels;S. Paltani;Arvind Parmer;R. Petre;M. Pohl;Scott Porter;B. Ramsey;C. Reynolds;S. Sakai;R. Sambruna;G. Sato;Yoichi Sato;P. Serlemitsos;M. Shida;T. Shimada;K. Shinozaki;P. Shirron;Randall K. Smith;G. Sneiderman;Y. Soong;L. Stawarz;H. Sugita;A. Szymkowiak;H. Tajima;H. Takahashi;Y. Takei;T. Tamagawa;T. Tamura;K. Tamura;Takaaki Tanaka;Yasuo Tanaka;Yasuyuki T. Tanaka;M. Tashiro;Y. Tawara;Y. Terada;Y. Terashima;F. Tombesi;H. Tomida;Miyako Tozuka;Y. Tsuboi;M. Tsujimoto;H. Tsunemi;T. Tsuru;H. Uchida;Y. Uchiyama;H. Uchiyama;Y. Ueda;S. Uno;M. Urry;S. Watanabe;N. White;Takahiro Yamada;H. Yamaguchi;K. Yamaoka;N. Yamasaki;M. Yamauchi;S. Yamauchi;Y. Yatsu;D. Yonetoku;A. Yoshida]
通讯作者：
Tadayuki Takahashi;K. Mitsuda;R. Kelley;F. Aharonian;F. Akimoto;S. Allen;N. Anabuki;L. Angelini;K. Arnaud;H. Awaki;A. Bamba;N. Bando;M. Bautz;R. Blandford;K. Boyce;G. Brown;M. Chernyakova;P. Coppi;E. Costantini;J. Cottam;J. Crow;J. Plaa;C. D. Vries;J. Herder;M. Dipirro;C. Done;T. Dotani;K. Ebisawa;T. Enoto;Y. Ezoe;A. Fabian;R. Fujimoto;Y. Fukazawa;S. Funk;A. Furuzawa;M. Galeazzi;P. Gandhi;K. Gendreau;K. Gilmore;Y. Haba;K. Hamaguchi;I. Hatsukade;K. Hayashida;J. Hiraga;K. Hirose;A. Hornschemeier;J. Hughes;U. Hwang;R. Iizuka;K. Ishibashi;M. Ishida;K. Ishimura;Y. Ishisaki;N. Isobe;Masayuki Ito;N. Iwata;J. Kaastra;T. Kallman;T. Kamae;H. Katagiri;J. Kataoka;S. Katsuda;M. Kawaharada;N. Kawai;S. Kawasaki;Dmitry Khangaluyan;C. Kilbourne;K. Kinugasa;S. Kitamoto;T. Kitayama;T. Kohmura;M. Kokubun;T. Kosaka;T. Kotani;K. Koyama;A. Kubota;H. Kunieda;P. Laurent;F. Lebrun;O. Limousin;M. Loewenstein;K. Long;G. Madejski;Y. Maeda;K. Makishima;M. Markevitch;H. Matsumoto;K. Matsushita;D. McCammon;Jonathan M. Miller;S. Mineshige;K. Minesugi;T. Miyazawa;T. Mizuno;K. Mori;H. Mori;K. Mukai;H. Murakami;T. Murakami;R. Mushotzky;Y. Nakagawa;T. Nakagawa;H. Nakajima;T. Nakamori;K. Nakazawa;Y. Namba;M. Nomachi;S. O. Dell;H. Ogawa;M. Ogawa;K. Ogi;T. Ohashi;M. Ohno;M. Ohta;T. Okajima;N. Ota;M. Ozaki;F. Paerels;S. Paltani;Arvind Parmer;R. Petre;M. Pohl;Scott Porter;B. Ramsey;C. Reynolds;S. Sakai;R. Sambruna;G. Sato;Yoichi Sato;P. Serlemitsos;M. Shida;T. Shimada;K. Shinozaki;P. Shirron;Randall K. Smith;G. Sneiderman;Y. Soong;L. Stawarz;H. Sugita;A. Szymkowiak;H. Tajima;H. Takahashi;Y. Takei;T. Tamagawa;T. Tamura;K. Tamura;Takaaki Tanaka;Yasuo Tanaka;Yasuyuki T. Tanaka;M. Tashiro;Y. Tawara;Y. Terada;Y. Terashima;F. Tombesi;H. Tomida;Miyako Tozuka;Y. Tsuboi;M. Tsujimoto;H. Tsunemi;T. Tsuru;H. Uchida;Y. Uchiyama;H. Uchiyama;Y. Ueda;S. Uno;M. Urry;S. Watanabe;N. White;Takahiro Yamada;H. Yamaguchi;K. Yamaoka;N. Yamasaki;M. Yamauchi;S. Yamauchi;Y. Yatsu;D. Yonetoku;A. Yoshida
DLC成膜によって曲げられたシリコン結晶の偏光X線特性評価
DLC成膜弯曲硅晶体的偏振X射线特性评价
DLC成膜弯曲硅晶体的偏振X射线特性评价
DOI：
--
发表时间：
2008
期刊：
影响因子：
--
作者：
[Aikawa, Y., 蜂巣泉, 坪井陽子,三角和由,戸塚晃太,赤坂大樹,大竹尚登,斎藤雅典]
通讯作者：
坪井陽子,三角和由,戸塚晃太,赤坂大樹,大竹尚登,斎藤雅典
DLC成膜によって曲げられたSi結晶の曲率とX線反射率
DLC膜形成弯曲Si晶体的曲率和X射线反射率
DLC膜形成弯曲Si晶体的曲率和X射线反射率
DOI：
--
发表时间：
2010
期刊：
影响因子：
--
作者：
[楠進吾, 武田誠也, 得能敦, 山室智史, 飯塚亮, 坪井陽子, 赤坂大樹, 大竹尚登, 斎藤雅典]
通讯作者：
斎藤雅典
The variable X-ray spectrum of the Wolf-Rayet binary WR140 with Suzaku
带有朱雀的沃尔夫-拉叶双星 WR140 的可变 X 射线光谱
带有朱雀的沃尔夫-拉叶双星 WR140 的可变 X 射线光谱
DOI：
--
发表时间：
2011
期刊：
Proceedings of the 39th Liège Astrophysical Colloquium
影响因子：
--
作者：
[Sugawara, Y., Maeda, Y., Tsuboi, Y., Hamaguchi, K., Corcoran, M., Pollock, A., Moffat, A., Williams, P., Dougherty, S., Pittard, J]
通讯作者：
J
An X-ray Study of a Massive Star and its Wind
大质量恒星及其风的 X 射线研究
大质量恒星及其风的 X 射线研究
DOI：
--
发表时间：
2010
期刊：
AIP Conference Proceedings
影响因子：
--
作者：
[Maeda, et al.]
通讯作者：
et al.
共 27 条
A Statistical Study of Protostars with Monitoring Observations in the X-ray Band
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批准号：23540269
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项目类别：Grant-in-Aid for Scientific Research (C)
-
资助金额：$3.16万
-
财政年份：2011
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负责人：TSUBOI Yohko
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依托单位：
海外基金