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    131. SAO Summer Intern Program Projects, 2010
    ... By limiting gas cooling, this "AGN feedback" can also regulate the rate of star ... of radio lobes to their observable properties in order to study AGN feedback ... the flow of matter and energy from the AGN and the host galaxy into the surrounding ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects10.html -- 22.4 Кб -- 01.10.2012
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    132. SAO Summer Intern Program Projects, 2010
    ... By limiting gas cooling, this "AGN feedback" can also regulate the rate of star ... of radio lobes to their observable properties in order to study AGN feedback ... the flow of matter and energy from the AGN and the host galaxy into the surrounding ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2010/projects10.html -- 22.7 Кб -- 01.10.2012
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    133. Intern Directory
    ... Berkeley . Reinout van Weeren . Lensed X-ray AGN . Samantha Scibelli . StonyBrook . ... Energetic processes in AGN . Colin Hill . MIT . Ken Rines . ... AGN heating of galaxies and groups . Conrad Hutcheson . U. Arizona . John Huchra . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~jcm/intern/intern.html -- 74.8 Кб -- 10.04.2016
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    134. http://hea-www.harvard.edu/~pgreen/vitanew_old/vitanew.ps
    ... in BALQSOs,'' P. J. Green 1997, in Mass Ejection in AGN, eds. N. Arav, I. Shlosman, & R. Weymann, (San Francisco: Astronomical ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/vitanew_old/vitanew.ps -- 199.7 Кб -- 15.01.2001
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    135. http://hea-www.harvard.edu/~kim/pap/2009_ChaMP_anca_apj.pdf
    ... nucleus (AGN) levels, there is an anticorrelation between and L/Ledd , opposite to the trend exhibited by high z AGN (quasars ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2009_ChaMP_anca_apj.pdf -- 1675.1 Кб -- 06.12.2010
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    136. http://hea-www.harvard.edu/~kim/pap/2012_N1291_Luo.pdf
    ... AGN has an intrinsic power-law photon index of 2 and an absorption column density of ... AGN Subtraction To derive the XLFs correctly, it is essential to make proper ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2012_N1291_Luo.pdf -- 990.9 Кб -- 30.08.2012
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    137. http://hea-www.harvard.edu/~pgreen/Papers/SDSSJ1004_06.pdf
    ... of absorber properties even more important to our understanding of AGN physics ... Given the wide ramifications for AGN physics, it is well worth considering. ... may well be qualitatively different from AGN outflows, but the dense line-driven ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/SDSSJ1004_06.pdf -- 567.6 Кб -- 13.10.2010
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    138. http://hea-www.harvard.edu/AstroStat/Stat310_1314/bc_20140408.pdf
    ... of time delay of line vs. continuum Past reverberation studies: Our SALT current campaign: Three z = 1 quasars - about 40 nearby AGN - about 10 z < 0.4 quasars - 7 distant objects but only 1 detection SALT setup: simulations Expected delay: 500 ­ 600 days ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1314/bc_20140408.pdf -- 927.1 Кб -- 07.04.2014
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    139. The AstroStat Slog 2007 July
    ... Principal component analysis has incorporated ratios of emission line-strengths for classifying Type-II AGN and star forming galaxies. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2007/07/page/2/index.html -- 21.7 Кб -- 02.03.2014
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    140. The AstroStat Slog Classification
    ... Principal component analysis has incorporated ratios of emission line-strengths for classifying Type-II AGN and star forming galaxies. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/classification/page/2/index.html -- 29.1 Кб -- 02.03.2014
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