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    1. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-172-c.pdf
    ... the solid component of the disks from sub-micron dust particles (typical of ISM) to ... Clearly the dust disk images can probe the dust properties as well as the disk ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-172-c.pdf -- 273.0 Кб -- 20.02.2013
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    2. http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02649v3.pdf
    ... a model of the physical dust temperature, because much of the disk does not have a ... However, further physical modeling of the disk dust continuum emission is needed to ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02649v3.pdf -- 401.3 Кб -- 04.03.2016
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    3. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/abstract_book.pdf
    ... Resonantly trapped rings of dust may be detected by the LBTI (for instance, the current HOSTS survey using LBTI is targeted to detect dust disks at ~10 times the level of the solar system's zodiacal light or greater) or in the future by JWST. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/abstract_book.pdf -- 124.5 Кб -- 09.04.2014
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    4. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/beautyAll.pdf
    ... Several source images were initially considered for the contest, including images of exozodiacal dust disks, contributed by Marc Kuchner (Princeton University), and images of jets from a Young Stellar Ob ject, contributed by Paulo Garcia (Universidade do ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/beautyAll.pdf -- 2044.2 Кб -- 20.02.2013
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    5. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/LMatra.pdf
    ... disks are generally considered gas-poor: most of the gas is expected to dissipate at ... disks, potentially providing key information to determine its provenance. " " (e.g ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/LMatra.pdf -- 1894.4 Кб -- 16.04.2014
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    6. Astrophysics Group Galaxy Formation and Evolution
    ... The starburst galaxy M82, which expels dust and metal enriched gas out of its disk . The Life Cycle of the ISM . ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/research/extragalactic-group-2/ -- 17.0 Кб -- 10.04.2016
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    7. http://www.mrao.cam.ac.uk/~cjld1/pages/geometryandcosmology2.pdf
    ... Dust =0 de Sitter phase Radiation =1/3 Initial singularity Cosmic Trajectories · For a range of initial conditions, models re-focus around the flat case · For decoupled matter and radiation can solve the equations exactly · Solutions governed by two ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~cjld1/pages/geometryandcosmology2.pdf -- 625.8 Кб -- 14.04.2004
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    8. http://www.mrao.cam.ac.uk/projects/aavp/presentations/Penny_SETI.pdf
    ... its sensitivity and resolution, the SKA will be able to observe the centimeterwavelength thermal radiation from dust in the inner regions of nearby proto-planetary disks and monitor changes as planets form, thereby probing a key regime in the planetary ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/aavp/presentations/Penny_SETI.pdf -- 1315.4 Кб -- 09.12.2010
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    9. High resolution studies of protostellar condensations in NGC 2024
    ... good candidates for the driving source of the CO outflow instead of radiation pressure, provided that a disk has already formed ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/wiesemeyer/wiesemeyer.html -- 25.3 Кб -- 08.12.2003
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    10. http://www.mrao.cam.ac.uk/~eic22/Papers/esma.pdf
    ... The density, temperature and velocity distribution of these disks critically determines the growth of dust particles, affects the chemistry and coagulation of planetesimals, and controls the gas accretion and orbital migration of massive planets. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~eic22/Papers/esma.pdf -- 1118.2 Кб -- 11.06.2009
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