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    11. http://www.mrao.cam.ac.uk/~eic22/Papers/esma.pdf
    ... These ob jects are likely to consist of the most unaltered matter from the Solar Nebula (see Ref. 3, and references therein), and are therefore essential to our understanding of the young Solar System. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~eic22/Papers/esma.pdf -- 1118.2 Кб -- 11.06.2009
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    12. Astrophysics Group Research and Instrumentation
    ... an extraordinary endeavour, in light of what we have learnt about Solar System planets, only a handful of key ingredients are ...
    [ 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/~bn204/almasim08/papers/64_50_presentaion_2008a.pdf
    ... we can track time changes to the same senstivity faster by (64/50)^2 = 1.64 Very fast mm variability is rare (solar flares ... Larger arrays will require some earth rotation synthesis to get complete coverage.The max config size for complete snapshop ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/almasim08/papers/64_50_presentaion_2008a.pdf -- 1160.4 Кб -- 02.12.2008
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    14. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/MROI_SPIE2006_Jurgenson_MROIsAutomatedAlignmentSystem.pdf
    ... made quad cells using space-qualified solar cells so that the centroiding errors can ... will be used here is an obstruction that rotates into the path of the laser, cocked ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/MROI_SPIE2006_Jurgenson_MROIsAutomatedAlignmentSystem.pdf -- 745.8 Кб -- 20.02.2013
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    15. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie7013-172-c.pdf
    ... Right: Expected rotation curve along the ma jor axis of a rotating gas disk in the nucleus of NGC 1365 for a disk inclination of i = 30 deg a BH mass of MBH 4 в 107 M and a distance of D 22 Mpc. ...
    [ 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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    16. Measurements of anisotropies in the Cosmic Microwave Background Radiation on
    ... mount causes the plane of polarization to rotate on the sky as the telescope tracks ... The observations were made at night to avoid solar interference. ... The rotation of the plane of polarization on the sky further reduces any unpolarized ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/osullivan/osullivan.html -- 19.8 Кб -- 08.12.2003
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    17. http://www.mrao.cam.ac.uk/yerac/osullivan/osullivan.ps
    ... mount causes the plane of polarization to rotate on the sky as the telescope tracks ... The observations were made at night to avoid solar interference. ... The rotation of the plane of polarization on the sky further reduces any unpolarized ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/osullivan/osullivan.ps -- 712.1 Кб -- 22.02.1995
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    18. http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02649v3.pdf
    ... the circumstellar disk surrounding the young solar analogue HL Tau, with a pattern ... as i = 0 for face-on), and rotated by an amount defined by the position angle (P.A ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02649v3.pdf -- 401.3 Кб -- 04.03.2016
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    19. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/mnr3438.pdf
    ... Fourier plane well, the aperture mask was rotated relative to the sky and 5000 short ... on 1.2 mm) of a model star with T eff 3750 KY log g 1X5 and solar composition ... coefficient of a model with T eff 3500 KY log g 0X5 and solar composition ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/mnr3438.pdf -- 449.7 Кб -- 20.02.2013
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    20. http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.Requirements/INT-402-MIS-0000.pdf
    ... The formation of solar-type stars and other `solar systems' is of obvious importance. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.Requirements/INT-402-MIS-0000.pdf -- 1989.2 Кб -- 25.06.2007
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