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    81. http://hea-www.harvard.edu/~elvis/Elvis_AGN_quasar_GCT_CFP.pdf
    ... How, and the quasar central engine work? do Supermassive Black holes grow? do quasars accelerate matter, up to the highest ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~elvis/Elvis_AGN_quasar_GCT_CFP.pdf -- 591.9 Кб -- 13.04.2011
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    82. http://hea-www.harvard.edu/~elvis/ref_papers.ps
    ... 40 1987 Quasar Energy Distributions: I. Soft X­ray Spectra of Quasars (B.J. Wilkes ... Quasar Luminosity Function from Accretion Disk In­ stabilities (A. Siemiginowska and ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~elvis/ref_papers.ps -- 73.3 Кб -- 13.04.2011
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    83. http://hea-www.harvard.edu/QEDT/Papers/joasia1.ps
    ... quasar spectra are generally believed to be generated in a large number of small gas clouds photoionized by the central ... the emission line properties are largely similar from quasar to quasar, the observed spectral energy distributions (SEDs) are ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/QEDT/Papers/joasia1.ps -- 275.7 Кб -- 03.09.1998
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    84. AstroStat Talks 2013-2014
    ... In quasars there is a physical link between the timescale and the absolute luminosity, so the key point in quasar application is to determine precisely the time delay between the continuum and the emission line in the optical band. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1314/ -- 37.4 Кб -- 10.04.2016
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    85. http://hea-www.harvard.edu/~pgreen/spitzer.pdf
    ... Quasars Sensitive, wide-area searches are required to find candidate mergers, and at ... quasar/galaxy connection, the properties of triggered AGN, and their environments ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/spitzer.pdf -- 307.5 Кб -- 10.03.2007
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    86. http://hea-www.harvard.edu/AstroStat/Stat310_fMMIV/siemiginowska_21sep2004.pdf
    ... The width of the lines => Velocity · Line location => Composition · Energy of the line => Temperature · Line variability => Distance from the Quasar Quasars Wind Hot outflowing wind, large distance from the center! ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMIV/siemiginowska_21sep2004.pdf -- 1933.7 Кб -- 25.07.2005
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    87. http://hea-www.harvard.edu/QEDT/Papers/pg1407.ps
    ... QUASAR PG1407+265 Jonathan C. McDowell 1 , Claude Canizares 3 , Martin Elvis 1 ... quasar: Prior to the detection of Hff, we had speculated that the object might not ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/QEDT/Papers/pg1407.ps -- 527.6 Кб -- 07.04.1995
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    88. http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/pty_20051024.pdf
    ... Statistical Model for the Spectrum Quasar PG 1634+706 PG 1634+706 is a redshift z=1.334 radio quiet and optically bright quasar ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/pty_20051024.pdf -- 840.5 Кб -- 25.10.2005
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    89. SAO Summer Intern Program Projects, 2012
    ... PROJECT TITLE: X-ray Emission in Luminous Quasars . Abstract: . ... This project concerns a sample of quasars observed in the optical and X-ray bands. ... the spectral energy distributions (SED) for the quasars using SDSS and Chandra (and ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2012/projects12.html -- 20.9 Кб -- 27.02.2014
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    90. http://hea-www.harvard.edu/~pgreen/SOC/2.html
    ... fitting and the morphological analysis of Quasar host galaxies for both classes of ... include (1) X-ray luminous, narrow-lined quasars; (2) X-ray bright, optically-normal ... X-ray properties of Spitzer-selected type-2 quasars . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~pgreen/SOC/2.html -- 15.3 Кб -- 01.10.2012
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