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    121. http://hea-www.harvard.edu/QEDT/Papers/ewol.ps
    ... AGN Aneta Siemiginowska 1;2 , Bo—zena Czerny 2 & Vadim Kostyunin 3 1 Harvard ... AGN both in spectral behavior and overall variability (Fiore & Elvis 1994, Tanaka ... center of AGN are not always in their active state so many low luminosity AGN may ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/QEDT/Papers/ewol.ps -- 826.4 Кб -- 28.08.1995
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    122. SAO Summer Intern Program Projects, 2007
    ... Active galactic nuclei (AGN) are among the most energetic astrophysical phenomena in ... of the energetic processes involved in AGN, through detailed studies of how jets ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/projects07.html -- 27.4 Кб -- 01.10.2012
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    123. AstroStat Talks 2014-2015
    ... into 4 categories: the AGN (Active Galactic Nuclei), which are divided into LINERs and Seyferts, the HII region-like galaxies(star forming galaxies) and the Composite galaxies (their spectra contain significant contributions from both AGN and star-forming ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1415/ -- 48.3 Кб -- 10.04.2016
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    124. http://hea-www.harvard.edu/~pgreen/BIQSOS/ChandraBiQSOs4.pdf
    ... When the AGN and/or starburst component contribution is estimated over the 1014 - 1018 Hz wavelength range, where we have available photometry, the luminosity of all 14 sources appears to originate mainly from an AGN component (>55%). ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/BIQSOS/ChandraBiQSOs4.pdf -- 472.9 Кб -- 24.03.2011
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    125. http://hea-www.harvard.edu/~kim/pap/2007_N821_II.pdf
    ... AGN (But Very Obscured ) We examine here the possibility that the nucleus of NGC 821 ... AGN flux is scattered into our line of sight and observed as source S2 with a L(2 Y ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2007_N821_II.pdf -- 280.3 Кб -- 06.12.2010
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    126. http://hea-www.harvard.edu/~pgreen/Papers/MassOutflow01.ps
    ... emission lines betray the presence of an AGN, the minimum di erence between our ... to clarify the relationship between merger/starburst activity and out ows in AGN ... a signi cant fraction of absorbed AGN postulated to contribute to the cosmic X-ray ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/MassOutflow01.ps -- 155.8 Кб -- 17.01.2002
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    127. The AstroStat Slog CMD
    ... 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/cmd/index.html -- 35.2 Кб -- 01.03.2014
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    128. http://hea-www.harvard.edu/~elvis/ref_papers.ps
    ... 1989 Accurate Galactic NH Values Toward Quasars and AGN (M. Elvis, F.J. Lockman, and ... 51 1990 A Highly X­ray Variable AGN: A Microlensing Candidate (G. Trinchieri, G ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~elvis/ref_papers.ps -- 73.3 Кб -- 13.04.2011
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    129. http://hea-www.harvard.edu/~kim/pap/RedQ_1999.pdf
    ... density of (blue) AGNs at B \ 21 is only D0.005 per error circle (e.g., Zitelli et al. 1992), we expect onlya1in4 chance of AGN coincidence in the 51 spectra, so stopping once an AGN is found will not produce a signiпcant number of false identiпcations ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/RedQ_1999.pdf -- 280.8 Кб -- 06.12.2010
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    130. http://hea-www.harvard.edu/~pgreen/Papers/postcos_04.pdf
    ... of the Astrophysical Journal Supplement. a AGN type: (Q) QSO, (Sy) Seyfert, (N LS 1 ... to the other components seen in AGN spectra: broad and narrow absorption lines, X ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/postcos_04.pdf -- 552.9 Кб -- 16.11.2004
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