Bursts from Soft Gamma-Ray Repeaters triggered by HETE-2

被引：0

作者：

Nakagawa, Y. E. ^{[1
]}

Maetou, M. ^{[1
]}

Yoshida, A. ^{[1
,2
]}

Sakamoto, T. ^{[3
]}

Suzuki, M. ^{[3
]}

Yamamoto, Y. ^{[3
]}

Tamagawa, T. ^{[1
,2
]}

Shirasaki, Y. ^{[2
,4
]}

Yamazaki, T.

Kawai, N. ^{[2
,3
]}

Matsuoka, M. ^{[5
]}

Fenimore, E. E. ^{[6
]}

Galassi, M. ^{[6
]}

Atteia, J. -L. ^{[7
]}

Hurley, K. ^{[8
]}

Ricker, G. ^{[9
]}

机构：

[1] Aoyama Gakuin Univ, Dept Phys, Sagamihara, Kanagawa, Japan

[2] RIKEN, Inst Phys & Chem Res, Wako, Saitama, Japan

[3] Tokyo Inst Technol, Dept Phys, Meguro Ku, Tokyo, Japan

[4] Natl Astron Observ Japan, Mitaka, Tokyo, Japan

[5] Japan Aerosp Explorat Agcy, Tsukuba, Ibaraki, Japan

[6] Los Alamos Natl Lab, Los Alamos, NM USA

[7] Observ Midi Pyrenees, Lab Astrophys, Toulouse, France

[8] UC Berkeley Space Sci Lab, Berkeley, CA USA

[9] MIT, Ctr Space Res, Cambridge, MA USA

来源：

NUOVO CIMENTO C-COLLOQUIA AND COMMUNICATIONS IN PHYSICS | 2005年 / 28卷 / 4-5期

关键词：

D O I：

暂无

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

HETE-2 triggered 166 events from SGR1900+14 and SGR1806-20 in summer periods from June 18 2001 to September 8 2004. Among these events, 6 events were localized to SGR1900+14 and 53 events to SGR1806-20. We performed the energy spectral analyses of bursts from SGR1900+14 and SGR1806-20 using the data of the WXM and FREGATE onboard HETE-2. Wefind that the energy spectra of SGR1900+ 14 and SGR1806- 20 are well described by a sum of two blackbody models with temperatures of similar to 4keVand similar to 11 keV.

引用

页码：625 / 628

页数：4

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