Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Stars: Individual: Alphanumeric: SGR 1900+14"'
Autor:
Yoshitaka Saito, N. Kawai, Toshifumi Mukai, Toshio Terasawa, Takeshi Takashima, Ichiro Yoshikawa, Yasuyuki T. Tanaka, A. Yoshida
Publikováno v:
The Astrophysical Journal Letters. 665(1):L55-L58
Accepted: 2007-06-20
資料番号: SA1000113000
資料番号: SA1000113000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::810f3ce082ab6571a837665c2b0ef4e0
http://id.nii.ac.jp/1696/00023450/
http://id.nii.ac.jp/1696/00023450/
Autor:
J. F. Olive, George R. Ricker, K. Hurley, N. Kawai, J. L. Atteia, C. Barraud, G. Crew, T. Sakamoto, G. Pizzichini
Publikováno v:
The Astrophysical Journal. 616:1148-1158
We present a detailed analysis of a 3.5 s long burst from SGR1900+14 which occurred on 2001 July 2. The 2-150 keV time-integrated energy spectrum is well described by the sum of two blackbodies whose temperatures are approximately 4.3 and 9.8 keV. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::18f72d0f83e014a3a30d603bdca245bd
https://doi.org/10.1086/424957
https://doi.org/10.1086/424957
Autor:
E. P. Mazets, Marco Feroci, S. V. Golenetskii, D. D. Frederiks, Chryssa Kouveliotou, Enrico Costa, Kevin Hurley, Marco Tavani, Sandro Mereghetti, Paolo Soffitta, P. M. Woods
Publikováno v:
596 (2003): 470–476.
info:cnr-pdr/source/autori:Feroci M. 1, Mereghetti S. 2, Woods P. 3., Kouveliotou C. 4, Costa E. 5, Frederiks D. D. 6, Golenetskii S. V. 7, Hurley K. 8, Mazets E. 9, Soffitta P. 10, Tavani M. 11/titolo:The 2001 April Burst Activation of SGR 1900+14: X-Ray Afterglow Emission/doi:/rivista:/anno:2003/pagina_da:470/pagina_a:476/intervallo_pagine:470–476/volume:596
info:cnr-pdr/source/autori:Feroci M. 1, Mereghetti S. 2, Woods P. 3., Kouveliotou C. 4, Costa E. 5, Frederiks D. D. 6, Golenetskii S. V. 7, Hurley K. 8, Mazets E. 9, Soffitta P. 10, Tavani M. 11/titolo:The 2001 April Burst Activation of SGR 1900+14: X-Ray Afterglow Emission/doi:/rivista:/anno:2003/pagina_da:470/pagina_a:476/intervallo_pagine:470–476/volume:596
After nearly two years of quiescence, the soft gamma-ray repeater SGR 1900+14 again became burst-active on April 18 2001, when it emitted a large flare, preceded by few weak and soft short bursts. After having detected the X and gamma prompt emission
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f2c231fd447d07ea33819b1e1bd67bb8
Autor:
Kawai, Nobuyuki
Publikováno v:
Astrophysical Journal. 510
The Advanced Satellite for Cosmology and Astrophysics (ASCA) observed the soft gamma repeater SGR 1900+14 on 1998 April 30-May 1 and discovered a pulsar with a period of 5.1589715(8) s from the known X-ray source of RX J190714.2+0919.3. Four months l
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=jairo_______::f03256e32a6e03a1cd4262232e866939
http://t2r2.star.titech.ac.jp/cgi-bin/publicationinfo.cgi?q_publication_content_number=CTT100551751
http://t2r2.star.titech.ac.jp/cgi-bin/publicationinfo.cgi?q_publication_content_number=CTT100551751