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    1. http://hea-www.harvard.edu/~kim/pap/BinaryQ_2002.pdf
    ... reproduce the observed distribution of projected separations of pairs but predict that binary quasars are only observable as such in the early stages of galactic collisions, after which the supermassive black holes would orbit within the merger remnant ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/BinaryQ_2002.pdf -- 1062.9 Кб -- 06.12.2010
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    2. http://hea-www.harvard.edu/~pgreen/Papers/um425_05.pdf
    ... They further suggest that binary quasars ``are only observable as such in the early stages of galactic collisions, after which the quiescent supermassive black holes orbit in the merger remnant for some time.' ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/um425_05.pdf -- 528.5 Кб -- 14.09.2005
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    3. http://hea-www.harvard.edu/~bradw/cv/papers/FeCX.pdf
    ... More importantly, because of the small CX cross sections at these high collision energies, CX line emission would be several orders of magnitude too weak to explain the Galactic plane emission. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/FeCX.pdf -- 351.9 Кб -- 15.11.2005
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    4. http://hea-www.harvard.edu/~bradw/cv/papers/FeCX.ps.gz
    ... More importantly, because of the small CX cross sections at these high collision energies, CX line emission would be several orders of magnitude too weak to explain the Galactic plane emission. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/FeCX.ps.gz -- 395.1 Кб -- 15.11.2005
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    5. QED Team - Papers
    ... The Spectral Energy Distributions of Active Galactic Nuclei", . ... Active Galactic Nuclei", . ... STAR-DISK COLLISIONS AND THE ORIGIN OF BROAD LINES IN QUASARS" . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/QEDT/TeamPapers.html -- 10.0 Кб -- 01.10.2012
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    6. dictionary
    ... When collisions occur between cosmic ray particles and atomic nuclei, gamma-rays are formed. Cosmic Rays . ... Image of the Trifid nebula . ACRONYMS . AGN . Active Galactic Nuclei . CV . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/CHAMP/EDUCATION/PUBLIC/dictionary.html -- 16.6 Кб -- 02.10.2012
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    7. http://hea-www.harvard.edu/~kim/pap/2012_N4649_Roberts.pdf
    ... 1) 785 8182 8507 12976 12975 14328 NH ,power law (2) <Galactic Galactic >Galactic Galactic >Galactic >Galactic MCD Fit Good ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2012_N4649_Roberts.pdf -- 608.2 Кб -- 24.04.2013
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    8. http://hea-www.harvard.edu/~bradw/cv/papers/maximBG.pdf
    ... Our results show, however, that even for these high Galactic latitude areas away from bright Galactic features, the line brightness varies significantly from field to field. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/maximBG.pdf -- 1015.8 Кб -- 13.01.2003
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    9. http://hea-www.harvard.edu/~kim/pap/2012_GCLMXB_theory.pdf
    ... The characteristic collision time for a binary is coll 0.8Gyr n5 a 100 v10 (Mbin + M ) (2) The total number of physical collisions (PCs) between RGs and NSs is NPC = nRG nNS RG,NS v , where nRG and nNS are the number densities of RGs and NSs accordingly ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2012_GCLMXB_theory.pdf -- 261.6 Кб -- 30.08.2012
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    10. http://hea-www.harvard.edu/~saku/papers.pdf
    ... 1991 The Einstein OGS Survey of Galactic Binary X-ray Sources (S.D. Vrtilek, J.E ... I. Collision Dominated Models (T.R. Kallman, S.D. Vrtilek, and S. Kahn), ApJ, 345 ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~saku/papers.pdf -- 78.9 Кб -- 01.10.2015
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