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    • [ В начало ] Пред. | 17 | 18 | 19 | 20 | 21 | 22 | 23 | 24 | 25 | 26 | След.

    221. The AstroStat Slog Spectral
    ... 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/category/spectral/page/2/index.html -- 55.3 Кб -- 02.03.2014
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    222. http://hea-www.harvard.edu/~kim/pap/2004_N507_XMM.pdf
    ... a low-luminosity active galactic nucleus (AGN ), not to mention some additional hard ... Some heating mechanisms (such as AGN feedback or thermal conduction) could ... is possibly related to the heating by the AGN, as indicated by the radio jet, or by ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2004_N507_XMM.pdf -- 1072.1 Кб -- 06.12.2010
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    223. http://hea-www.harvard.edu/~elvis/vigorous.pdf
    ... agn etosphe r e X - r a y sp e c t r a l p h e n o m e n a o f stella r and g ala ctic systems Plasma physics, au ro r a Sola r co r on a, IPM, ISM, cosmic r a ys Nitric oxide d ensity fluctu ations in the rmosphe r e du e to sola r and au ro r al a ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~elvis/vigorous.pdf -- 359.4 Кб -- 14.04.2011
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    224. http://hea-www.harvard.edu/~kim/pap/2006_ChaMP_cluster.pdf
    ... follow-up was optimized to probe AGN counterparts and not faint galaxies at a ... cluster (600 ) X-ray source (3000 ) AGN (1200 ) Galaxy cluster (000 ) Galaxy cluster ... within them and were targets of the ChaMP spectroscopic AGN follow-up program ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2006_ChaMP_cluster.pdf -- 798.6 Кб -- 06.12.2010
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    225. http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.pdf
    ... loBAL QSOs may contain at best very weak active galactic nuclei (AGN) and are instead dominated by massive starbursts (see, e.g ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.pdf -- 161.6 Кб -- 14.09.2005
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    226. http://hea-www.harvard.edu/~elvis/extreme_SPIE06.pdf
    ... 2006); · AGN wind location and characterization using non-equilibrium modelling of 'Warm Absorbers' (Krongold et al., 2006); · spectral Doppler mapping of the nearest several supernova remnants, galaxies and clusters of galaxies; · thermonuclear burning ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~elvis/extreme_SPIE06.pdf -- 128.1 Кб -- 13.04.2011
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    227. http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.ps
    ... loBAL QSOs may contain at best very weak active galactic nuclei (AGN) and are instead dominated by massive starbursts (see, e.g ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/chandrabals01.ps -- 694.8 Кб -- 14.09.2005
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    228. http://hea-www.harvard.edu/~jcm/asc/docs/ps/SDS01.ps
    ... Irr, Sa, Sb, Scd, S0, E, starburst; Groups, clusters of galaxies; AGN and quasars by sub­classes BL Lacs, Seyferts, + others ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~jcm/asc/docs/ps/SDS01.ps -- 242.9 Кб -- 03.04.1998
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    229. http://hea-www.harvard.edu/vlp_m33_public/ic131_102909.pdf
    ... Although the photon index and the hardness ratios for FL073 could also indicate an AGN, the column density suggests that this object is part of IC131-se and is likely not a background AGN. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/vlp_m33_public/ic131_102909.pdf -- 1615.2 Кб -- 29.10.2009
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    230. http://hea-www.harvard.edu/QEDT/Papers/lbqs.ps
    ... Zimmerman, H.­U., Staubert, R. 1992,, in X­ray Emission from AGN and the Cosmic X­ray Background, eds. W. Brinkmann, & J. Tr ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/QEDT/Papers/lbqs.ps -- 195.2 Кб -- 11.08.1995
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