... eclipses Discussion and conclusions December 26, 2007 HEA-2007 2 of 23 INTRODUCTION ... eclipses primary max. crossover I Several orbital eclispses were observed at ... eclipsed by the star and disk bodies December 26, 2007 HEA-2007 13 of 23 s Joint ...
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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
... of eclipse of the X-ray source by the normal star and in the middle of the eclipse ... of eclipses; the bottom panel: minimum flux at the middle of eclipses crossover ...
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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
... results of Vela X-1, an eclipsing neutron star hosted in a windaccreting high-mass X ... source in the region is Vela X-1, an eclipsing wind accreting high-mass X-ray binary ... 5. VELA X-1 PERSISTENT AVERAGE SEPCTRA Eclipses Fig. 3. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G46_Schanne01-05Jan07_17:47:00_bandw.pdf -- 482.8 Кб -- 10.01.2007 Похожие документы
... results of Vela X-1, an eclipsing neutron star hosted in a windaccreting high-mass X ... source in the region is Vela X-1, an eclipsing wind accreting high-mass X-ray binary ... 5. VELA X-1 PERSISTENT AVERAGE SEPCTRA Eclipses Fig. 3. ...
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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
... also performed during disk eclipses -- a total of three eclipses were observed in ... panel -- out of the eclipses of accretion disk, lower panel -- during the eclipse ...
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Ссылки http://hea.iki.rssi.ru/rtt150/en/ss433_pazh10/pss433_fast_a.pdf -- 531.9 Кб -- 12.01.2011 Похожие документы
... The solid line on top of the JEM-X light curve represents the ASM RXTE light curve averaged over many 35 d cycles and stretched vertically to match the one from JEM-X. Pre-eclipse dips (sharp flux decrease just before the eclipse) are clearly seen. ...
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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
... It is achieved when the blob eclipses the whole jet, i.e. rc . ... In the extreme case, when the blob eclipses the entire jet (i.e. 2 2 /rc 1), this scale depends only on the jet Lorentz factor ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/22/Barkov.pdf -- 1990.9 Кб -- 26.01.2011 Похожие документы
... These numbers are very similar to those estimated from the partial eclipse depth (50 %) of the hard X-ray light curves ... Due to the lack of a total eclipse the inclination can not be much larger than 60 degrees. ...
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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