... spectrum measured by RXTE/PCA from the XTEJ1901+014 position (scaled by a factor of 2 for clarity); b) Reconstructed true ... we can just renormalized this spectrum (using the scan data) to get the Galactic ridge spectrum at the XTEJ1901+014 position ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/E30_Karasev01-27Mar07_15:40:32.pdf -- 209.0 Кб -- 18.06.2007 Похожие документы
... spectrum decreases as ( ) -2 Is it always correct that ... the apparent brightness of an off-axis jet decreases as L ~ ( ) -6 No No the peak (cut-off) frequency in the spectrum decreases as ( ) -2 Is it always correct that ... the apparent brightness of ...
... Hardening of the X-ray spectrum at the disk entrance and subsequent softening on a ... of disk entrance would result in hardening of the X-ray spectrum on a day scale ... Absence of the break in the X-ray spectrum favors the "hidden pulsar" model. ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/presentations.orig/26.12.07/chernyakova.pdf -- 1298.5 Кб -- 29.12.2007 Похожие документы
... energy cosmic rays by cluster accretion shocks V.S. Ptuskin, S.I. Rogovaya, V.N. Zirakashvili IZMIRAN HEA-2007 all-particle spectrum of cosmic rays at the Earth modulation by solar wind E -2 .7 E -3 .1 GZK energy losses of ultra-high energy cosmic rays in ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2007/presentations/25.12.2007/03-ptuskin.pdf -- 562.9 Кб -- 30.01.2008 Похожие документы
... Softening (hardening) of the X-ray spectrum on a day scale in the disk. ... 10 MeV at the disk the X-ray spectrum on a day scale. energy photons, leading to the ... to the hard X-ray synchrotron spectrum due to the inefficiency of the synchrotron ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2008/Presentations/24Dec/Chernyakova_IKI2008.pdf -- 1084.9 Кб -- 16.01.2009 Похожие документы
... complicates the analysis of the spectrum LIST OF THE SPECTRA · · · · · · · · · 3-5 ... BTA spectra SNR/px 2000 MODEL ATMOSPHERES · Spectrum analysis was made for the model ...
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Ссылки http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Balega.pdf -- 453.0 Кб -- 26.01.2011 Похожие документы
... The overall energy spectrum extends up to 150 keV and is well described by a ... The spectrum was well described by a disk-blackbody and a comptonization (CompTT ... Data and model of the spectrum are reported in Fig. 3, while in Table 1 are reported ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G35_Tarana02-27Apr07_13:29:31.pdf -- 144.9 Кб -- 27.04.2007 Похожие документы
... spectrum on the source's state for pulsars with variable fluxes: if the spectrum did ... spectrum averaged over all outbursts and an average persistent spectrum outside the ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G39_Filippova01-23Jan07_14:14:00.pdf -- 273.5 Кб -- 23.01.2007 Похожие документы
... 4.1 Average Spectrum The average sum-spectrum was fitted with the DISKBB+COMPBB model between 3 100 keV _____________________________________________________________________ Proc. 6th INTEGRAL Workshop `The Obscured Universe', Moscow, 3-7 July 2006 (ESA ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G31_Hjalmarsdotter03-17Apr07_14:14:42.pdf -- 251.4 Кб -- 17.04.2007 Похожие документы
... had been proposed ([3]), we first took a spectrum of the only star within the error ... The spectrum corresponds to an M type star, with pronounced TiO molecular bands (Fig ... In Fig. 2 we show the spectrum in the classification region. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G52_Torrejon01-26Apr07_13:48:22.pdf -- 108.1 Кб -- 26.04.2007 Похожие документы