... The best-fit parameters are 0 = 9.6 M kpc-3 , RS = 11.1 kpc, and M/LV = 4.5. ... 12 rate is MB = 0.046 M yr-1 for = 5/3 (as adopted hereafter; MB would be 4.5 times ...
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Ссылки http://hea-www.harvard.edu/~kim/pap/2014_N4649_AGNfeedback.pdf -- 1400.2 Кб -- 19.10.2014 Похожие документы
... similar accuracy on scales as small as 5 Їm. Together, the HXDS detectors provide a ... designed for grating and Ring Focus measurements), ranging between 5 and 500 Їm wide ...
... 9.1 9.2 9.4 9.6 2 2 4 6 8 Sun 2 4 6 8 Sun 2 4 6 8 Sun True Initial Mass (M ) True Initial Mass (M ) True Initial Mass (M ) 95% Posterior Intervals (M Sun ) 0.5 1.0 1.5 0.5 1.0 1.5 Sun 0.5 1.0 1.5 Sun 0.5 1.0 1.5 Sun True Final Mass (M ) True Final Mass (M ...
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Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1213/nms_20120904.pdf -- 1424.4 Кб -- 04.09.2012 Похожие документы
... infrared (IR) through soft Xray (100 Їm -- 3.5 keV) continuum data for a sample of ... 1704+608 (L(0.81.6Їm)?45.5) and those that contributed to the low luminosity mean ...
... rate associated with CMEs is at least ?5 25оТ 10Р14 M yrР1, but it may well be ... YZ CMi has an optically thick wind and loses mass at the rate of $5 Т 10Р10 ` M yrР1 ...
... X-RAY ABSORPTION IN A BROAD ABSORPTION LINE QUASAR, PG 0946 301 S. Mathur,1,2 P. J. Green,2 N. Arav,3 M. Brotherton,4 M. Crenshaw,5M. deKool,6 M. Elvis, R. W. Goodrich,7 F. Hamann,8 D. C. Hines,9 V. Kashyap,2 K. Korista,10 B. M. Peterson,1 J. C. Shields ...
... of our optical spectra with the WIYN 3.5m and CTIO 4 m with the HYDRA multifiber ... We have been using the FLWO 1.5m to acquire spectra of the optically bright (r 0 ...
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Ссылки http://hea-www.harvard.edu/~kim/pap/2005_ChaMP_hard_AGN.pdf -- 1020.4 Кб -- 06.12.2010 Похожие документы
... RAY ABSORPTION IN A BROAD ABSORPTION LINE QUASAR, PG 0946#301 S. Mathur, 1,2 P. J. Green, 2 N. Arav, 3 M. Brotherton, 4 M. Crenshaw, 5M. deKool, 6 M. Elvis, 2 R. W. Goodrich, 7 F. Hamann, 8 D. C. Hines, 9 V. Kashyap, 2 K. Korista, 10 B. M. Peterson, 1 J ...