... On one hand, we have seen that the spectral state of the source changes from a softer spectrum during the BS to a harder spectrum during the FS, with the possible presence of an intermediate state during the transition from BS to FS. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G48_Blay02-16Feb07_17:46:51.pdf -- 264.3 Кб -- 16.02.2007 Похожие документы
... galactic microquasar with hard X-ray spectrum (Cherepashchuk et al 2003) December 26 ... the unchanged shape of the X-ray spectrum over precessional period and broad X-ray ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/presentations/26.12.2007/02-cherepashchuk.pdf -- 1364.2 Кб -- 30.01.2008 Похожие документы
... 55), the spectrum reaches 360 keV and is well reproduced by a pure thermal model (Comptt [13] or Compps [10]) (but with the suspicion of the presence of a hard tail), while during the first plateau phase of the LHS (Rev. 57), the SPI spectrum reaches 500 ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/E39_Deluit01-28Feb07_19:42:02.pdf -- 1090.1 Кб -- 28.02.2007 Похожие документы
... The observed spectrum thus exhibits absorption features at the line energies: 1 ... profiles for a flat input continuum spectrum, when allowing scattering processes off ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G41_Schoenherr01-07Feb07_16:54:04.pdf -- 385.0 Кб -- 07.02.2007 Похожие документы
... spectrum gives a reasonable fit at radio frequencies, going through the optical ... spectrum gives emission in x-ray frequencies, and the second order inverse Compton ... spectrum gives emission in the x-ray frequencies, and the second order spectrum ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/D37_Tsang01-08Feb07_19:28:05.pdf -- 131.8 Кб -- 08.02.2007 Похожие документы
... On the other hand, the 2127 keV line from the decay of Cl ( =32 minutes) is not observed in the experimental spectrum, whereas it is relatively strong in the simulated spectrum of Fig. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B38_Tatischeff01-14Feb07_12:46:42.pdf -- 67.8 Кб -- 14.02.2007 Похожие документы
... spectrum of Her X-1 (best fit model parameters with 1 uncertainties are shown); middle panel: residuals after fitting the ... AVERAGED SPECTRUM For constructing the average spectrum, we used the data from revolutions 339 and 340. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G42_Klochkov01-05Feb07_15:40:11.pdf -- 173.0 Кб -- 05.02.2007 Похожие документы