... in the optical, medium X-ray, hard X-ray, and gamma spectral region (or at least a ... X-ray spectra (hot white dwarfs?), group b: harder X-ray spectra (colliding winds ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G53_Hudec02-16Feb07_17:12:18.pdf -- 540.7 Кб -- 16.02.2007 Похожие документы
... 5]) whose wind feeds the accretion luminosity 1038-39 erg/s from radio to X-rays ([3 ... displays a 4.8 hour modulation in X-rays and IR which can be assumed to be due to ...
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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
... 5]) whose wind feeds the accretion luminosity 1038-39 erg/s from radio to X-rays ([3 ... displays a 4.8 hour modulation in X-rays and IR which can be assumed to be due to ...
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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
... of a new hard X-ray outbursts of the transient X-ray binary pulsar GS1843+009 with ... X-ray radiation from the shock due to wind-wind collision and interpret the X-ray ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G51_Seifina01-12Dec06_03:14:40.pdf -- 496.4 Кб -- 12.12.2006 Похожие документы
... X-rays in the range 10 - 200 keV does not change with the precessional phase which ... X-ray binary at an advanced evolutionary stage has been investigated in optical ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/F03_Cherepashchuk01-06Feb07_17:34:47.pdf -- 424.7 Кб -- 06.02.2007 Похожие документы
... the best-ever spectral coverage in UV-, X-ray -, and hard X-ray energies was derived ... at X-ray (top: Swift/XRT 0.210 keV) and hard X-ray (bottom: INTEGRAL/ISGRI: 2060 keV ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/D35_Collmar01-27Feb07_19:21:51.pdf -- 260.7 Кб -- 27.02.2007 Похожие документы