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    1. Strong Gravity in the Vicinity of Supermassive Black Holes - by Eamon Scullion,
    ... Active Galactic Nuclei form in the accretion disks of supermassive black holes and ... simulations to model emission from accretion disks around such supermassive black ... over all angles between the observed accretion disk, with an inclination of 35 ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/scholars/iya/news/strong_gravity_in_the_vicin.html -- 12.2 Кб -- 31.12.2009
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    2. Lindsay Symposium
    ... Tom Ray, Dublin Institute for Advanced Studies . "Accretion Disks and Outflows Around Brown Dwarfs". ... Recent studies have shown that young brown dwarfs, like young stars, may be surrounded by accretion disks. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/lindsay/presentations/Ray.html -- 4.2 Кб -- 07.02.2007
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    3. Homepage of Gavin Ramsay
    ... They suggested the 4 hr period was a signature of an orbital period; the longer period was possibly due to precession of an accretion disk and KIC 9202990 was a cataclysmic variable with an accretion disk which is always in a bright state (a nova-like ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~gar/ -- 3.3 Кб -- 23.11.2015
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    4. http://star.arm.ac.uk/preprints/2012/607.pdf
    ... We detect eclipses of the accretion disk by the mass donating secondary star every 3.74 hrs which is the binary orbital period. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2012/607.pdf -- 747.1 Кб -- 05.07.2012
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    5. http://star.arm.ac.uk/preprints/2009/542.pdf
    ... material can be determined from accretion disk spectra (Fig. 1) and often can be ... or C/O rich, e.g. Fig. 1), accretion disk theories developed for H-rich gas can be ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2009/542.pdf -- 291.3 Кб -- 18.02.2009
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    6. http://star.arm.ac.uk/research/iaj-unify.ps
    ... is more or less complete, bringing in the accretion disk and envelope evolutions ... The gas reaches an inner accretion disk at the same rate as with which it is ... disk can be found by requiring the disk accretion time scale tљ (R) = R 2 =љ to be ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/research/iaj-unify.ps -- 1486.9 Кб -- 03.11.2005
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    7. Armagh Observatory
    ... They suggested the 4 hr period was a signature of an orbital period; the longer period was possibly due to precession of an accretion disk and KIC 9202990 was a cataclysmic variable with an accretion disk which is always in a bright state (a nova-like ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2015/682.html -- 6.0 Кб -- 02.11.2015
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    8. http://star.arm.ac.uk/preprints/2015/682.pdf
    ... the longer period was possibly due to precession of an accretion disk and KIC 9202990 was a cataclysmic variable with an ... would then give rise to negative sup er-humps since the accretion disk bright sp ot should sweep first across one face of the ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/2015/682.pdf -- 1652.3 Кб -- 02.11.2015
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    9. Armagh Observatory
    ... Tom Ray, Dublin Institute for Advanced Studies . "Accretion Disks and Outflows Around Brown Dwarfs". ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/lindsay/media/Ray.html -- 4.4 Кб -- 29.07.2013
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    10. Armagh Observatory
    ... We detect eclipses of the accretion disk by the mass donating secondary star every 3.74 hrs which is the binary orbital period. ... disk radius due to the presence of high viscosity material associated with the outburst, followed by a contraction in ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/highlights/2012/607.html -- 5.7 Кб -- 05.07.2012
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