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Ссылки http://hea-www.harvard.edu/AstroStat/HEAD2004/poster_sourlas.pdf -- 486.2 Кб -- 20.09.2004 Похожие документы
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... 2 Т 10Р15 ergs sР1 cmР2 resulted in a slope of the cumulative log N log S М 0:67 Ц 0:14, which is again in good agreement with our data ( М 0:7 Ц 0:15 for a single power-law fit at fX < 5 Т 10Р15 ergs sР1 cmР2; note that М Р 1 does not hold below Sbreak ...
... The X-ray investigation shows a hard (Р М 1:89) and moderately absorbed (NH М 1:8 Т 1021 cmР2 ) nuclear source of 1:5 Т 1040 ergs sР1 in the 2-10 keV band, surrounded by hot gas at a temperature of $0.6 keV. ...
... The effect of varying the source model between reasonable power-law Gal slopes from Р М 1:0 to 2.5 causes ( for NH М 3 Т 1020 cmР2) an increase in the derived fX (0.5 - 2 keV) of $ 12% for FI chips, and 6% for BI chips. ...
... the total flare-related mass loss was between 2:7 Т 10Р13 and 4:4 Т 10Р10 M yrР1 ... Т 106 K; log T М 6:56), is slightly cooler than the 6:1 Т 106 K obtained from the ... Т 10Р14 M yrР1, where 33 g. With abundance ratios of 0.044 for He relM is 2 Т 10 ...
... For comparison with work by Cravens et al. (2001) and RobeP Р & Cravens (2003a), we calculate the value of rtson С М il ni =np ... Robertson & Cravens (2003a) estimate that equals 6 Т 10Р16 eV cm2 for CT with H and 3 Т 10Р16 eV cm2 for He. ...