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    81. http://www.mrao.cam.ac.uk/~krause/Krause2002a.ps.gz
    ... mass would be { at any evo- lutionary state, the systems are observed at so far { in cold fragments just about to form stars ... The Jeans mass in the shell is  10 6 10 7 M . Hence, the shell will form stars in globular clusters of that mass. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~krause/Krause2002a.ps.gz -- 78.1 Кб -- 14.02.2005
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    82. John Young's Home Page
    ... Surface asymmetries on evolved stars ( example results ) . ... Stellar pulsation and mass loss . Fundamental parameters of stars . ... Stellar pulsation and mass loss . Fundamental parameters of stars . ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~jsy1001/ -- 4.5 Кб -- 12.02.2014
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    83. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/ABarker1.pdf
    ... Model is also relevant for terrestrial planets with deep oceans and Neptune/Uranus-mass planets, and to convective envelopes of stars] Ogilvie 2009 Favier, Barker, Baruteau & Ogilvie, 2014, MNRAS Topic 2 Tides in rotating planets with a core · Simplified ...
    [ 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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    84. http://www.mrao.cam.ac.uk/galevol/tgreve.pdf
    ... 3 1% 10 pc 1 kpc Krumholz+10 Sunday, October 6, 2013 star formation (IR-CO) relations at high redshifts Challenges: · Size measurements are difficult · CO-to-H2 gas mass conversion dubious Extended ~ 10 pc scales low density ~ 10 -10 cm · · · · · Greve+05 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/galevol/tgreve.pdf -- 2211.6 Кб -- 07.10.2013
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    85. http://www.mrao.cam.ac.uk/~anthony/latex/Hirashita.ps
    ... the in- formation on the star formation history of dSphs, we investigate the relation between their metallicity and virial mass ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~anthony/latex/Hirashita.ps -- 23.6 Кб -- 22.06.2000
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    86. http://www.mrao.cam.ac.uk/galevol/Cambridge2013_Yabe_v2.pdf
    ... Mass-Metallicity Relation up to z~3 · Gas-phase metallicity (hereafter, metallicity) Metallicity is a key to understand the ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/galevol/Cambridge2013_Yabe_v2.pdf -- 1807.4 Кб -- 07.10.2013
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    87. http://www.mrao.cam.ac.uk/galevol/salberts_cambridge_conference.pdf
    ... local Universe are generally red and dead. increased star forming fraction toward cluster cores at z>1.4 (e +10, Tran+10, Hayashi+11, Fassbender+11) .g. Hilton m* evolution of 4.5um luminosity function of cluster galaxies -> rapid mass assembly at z>1.3 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/galevol/salberts_cambridge_conference.pdf -- 2035.6 Кб -- 06.10.2013
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    88. http://www.mrao.cam.ac.uk/~jsy1001/thesis.pdf
    ... radius which contains all but an arbitrary small fraction of the mass of the star ... the interstellar medium, and the final mass of the star determines its ultimate fate ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~jsy1001/thesis.pdf -- 2354.4 Кб -- 20.07.1999
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    89. Astrophysics Group COAST
    ... The MROI will provide new insights into the physics of star and planet formation, stellar accretion and mass loss, and Active Galactic Nuclei. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/outreach/radio-telescopes/coast/ -- 17.9 Кб -- 10.04.2016
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    90. http://www.mrao.cam.ac.uk/secure/amiday/white_paper/AMI_Operations_science_case.pdf
    ... dynamic range, this band offers a unique window on numerous vital physical processes including, but not limited to, the formation of stars in both the high and low mass regimes, as well as the earliest stages of planet formation from circumstellar disks ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/secure/amiday/white_paper/AMI_Operations_science_case.pdf -- 59.5 Кб -- 10.08.2012
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