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    11. Astrophysics Group Program and talks
    ... Haswell Carole . 14:15 . A6 . Deep-atmosphere, non-hydrostatic models of hot Jupiter atmospheres. Mayne Nathan . 14:30 . A7 . ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/research/exoplanets/meetings/past-meetings/exo-meeting-2014/program/ -- 31.9 Кб -- 10.04.2016
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    12. Astrophysics Group Research and Instrumentation
    ... Orbital phase curve of the hot Jupiter exoplanet Kepler-7b, observed by the Kepler spacecraft (black points). ... curve (as the planet revolves around its star) of the hot-Jupiter Kepler-7b obtained from 3.5 years quasi continuous data from ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/research/exoplanets/research/ -- 22.7 Кб -- 10.04.2016
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    13. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/ABarker1.pdf
    ... Anomalously large radii of some HJs may partly be explained by tidal heating in the planet Orbital evolution of Jupiter/ Saturn satellites (Lainey et al, 2009,2012) due to tides Mercury Adrian Barker DAMTP, Cambridge Introduction Tide in planet m? = mp Rp ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/ABarker1.pdf -- 2342.7 Кб -- 17.04.2014
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    14. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/AHall-P.pdf
    ... These are represented in Figure 7, and show how, even with a limited dataset comprising of 30 nights, we have 53 candidates consistent with a transiting companion with twice Jupiter's radius or less. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/AHall-P.pdf -- 2664.7 Кб -- 16.04.2014
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    15. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/AMustill.pdf
    ... mass and radius from the SSE stellar models4 In Veras et al. (2013) we studied the evolution of systems of two Jupiter-mass planets separated by a range of separations We restricted attention to stars >=3M to avoid the computational S ol cost of long MS ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/AMustill.pdf -- 500.2 Кб -- 23.04.2014
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    16. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/DForgan.pdf
    ... on our previous 1D latitudinal energy balance models (LEBMs) which evolves the latitudinal temperature Subhead Body Text bution on an Earth-like moon orbiting a Jupiter-like distri planet, which in turn orbits a Sunlike star (Forgan and Kipping 2013 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/DForgan.pdf -- 1126.0 Кб -- 16.04.2014
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    17. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/HOsborn.pdf
    ... Introduction Nearly all of the ~200 transiting exoplanets discovered from the ground are larger than Jupiter and orbit with short periods (<11 days). ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/HOsborn.pdf -- 292.9 Кб -- 16.04.2014
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    18. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/MNeveu.pdf
    ... Surveyed Southern Wasp planets. The X axis is the hot Jupiter's period. The Y axis is the host star's temperature. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/MNeveu.pdf -- 586.3 Кб -- 17.04.2014
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    19. http://www.mrao.cam.ac.uk/~pjds/ascript/users/orbits.txt
    ... s1=mercury) set_character(c1,Y) end_if if (s1=venus) set_character(c1,Y) end_if if (s1=mars) set_character(c1,Y) end_if if (s1=jupiter) set_character(c1,Y) end_if if (s1=saturn) set_character(c1,Y) end_if if (s1=uranus) set_character(c1,Y) end_if if (s1 ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~pjds/ascript/users/orbits.txt -- 2.3 Кб -- 12.10.1996
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    20. http://www.mrao.cam.ac.uk/~pjds/ascript/users/realtime.txt
    ... s1=mercury) set_character(c1%p) end_if if (s1=venus) set_character(c1%p) end_if if (s1=mars) set_character(c1%p) end_if if (s1=jupiter) set_character(c1%p) end_if if (s1=saturn) set_character(c1%p) end_if if (s1=uranus) set_character(c1%p) end_if if (s1 ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~pjds/ascript/users/realtime.txt -- 3.4 Кб -- 12.10.1996
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