... resonant scattering features (CRSF) in the average spectrum of Vela X-1 has been ... We derive the persistent average spectrum of Vela X-1, using JEM-X and ISGRI, by ... 8. JEM-X, ISRGI and SPI persistent average spectrum of Vela X-1 (combined fit). ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G46_Schanne01-05Jan07_17:47:00_color.pdf -- 396.8 Кб -- 10.01.2007 Похожие документы
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... a model spectrum using the XSTAR-code and compare it with a Chandra spectrum ... spectrum The simulations also predict a nice agreement with the Chandra-spectrum ... spectrum (solid line, dereddened by NH = 5 x 1022 cm-2 ) and corresponding model ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/F39_Hjalmarsdotter02-17Apr07_14:19:21_bandw.pdf -- 212.8 Кб -- 17.04.2007 Похожие документы
... a model spectrum using the XSTAR-code and compare it with a Chandra spectrum ... spectrum The simulations also predict a nice agreement with the Chandra-spectrum ... spectrum (black line, dereddened by NH = 5 x 1022 cm-2 ) and corresponding model ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/F39_Hjalmarsdotter02-17Apr07_14:19:21_color.pdf -- 192.4 Кб -- 17.04.2007 Похожие документы
... SPECTRUM blue, red and black lines present power spectra of reprocessing function ... 2008) Composite spectrum of Cyg X-2 EXOSAT-ASM-PCA (RXTE) power spectrum of Cyg X-2 ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Titarchuk.pdf -- 1854.0 Кб -- 26.01.2011 Похожие документы
... 511 keV line from the X-ray Nova Muscae: . spectrum . sky image in the 511 kev line (180K) . ... SIGMA spectrum of the "Great Annihilator" 1E1740-294 . List of publications (69) can be found here . Links . ...
... 511 keV line from the X-ray Nova Muscae: . spectrum . sky image in the 511 kev line (180K) . ... SIGMA spectrum of the "Great Annihilator" 1E1740-294 . List of publications (69) can be found here . Links . ...
... 15 200 100 1300 100 1400 1500 Time (s) 1600 measured spectrum simulated spectrum 1700 Counts 10 1 0.1 0 100 200 300 Energy (keV ... Because of the evolution of the GRB spectra, the combined spectrum is slightly softer than the spectrum of R1. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/I32_Kalemci01-14Feb07_17:25:59_color.pdf -- 115.6 Кб -- 14.02.2007 Похожие документы