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    1. Simon Jeffery's Research: Molecules and Dust
    ... In the outermost layers of stars - especially cool stars - and in interstellar space, temperatures become very low and conditions are favourable for atoms to combine as molecules and for molecules to aggregate as grains of dust. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/research/dust.html -- 4.9 Кб -- 12.06.2002
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    2. Armagh Observatory
    ... Ambipolar diffusion: the magnetic field is not tied to the molecules. ... ions drift or stream through the neutral molecules, then the field can be released ... C-shocks is observed as infrared and submillimeter radiation from excited molecules ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/research/ambipolar.html -- 7.6 Кб -- 08.03.2013
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    3. M.D. Smith, Research Astronomer
    ... A collapse or implosion of a cloud of gas containing molecules and dust may lead to a low-mass star like our Sun. ... This leaves us with new questions: how can molecules survive such shattering speeds, and how do the cloud and protostar ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep99/node14.html -- 10.4 Кб -- 05.05.2000
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    4. Armagh Observatory
    ... The emission is from hydrogen molecules, at a rest wavelength of 2.12 microns. ... the same model paraboloidal bow, C-type (i.e. the molecules are excited by the friction with streaming ions), shown moving at ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/research/bows.html -- 4.9 Кб -- 08.03.2013
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    5. M.D. Smith, Research Astronomer
    ... It turns out that the field can gradually slip out of the denser clumps of molecules by a process called ambipolar diffusion (a decoupling process: charged ions become rare, and the neutral molecules then slip between them). ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep98/node14.html -- 9.2 Кб -- 14.12.1999
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    6. Armagh Observatory
    ... What kind of atoms make up the molecules that make up the cells that make our bodies? ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/publicevents/Robinson-Schools-2004.html -- 5.6 Кб -- 19.08.2011
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    7. Armagh Observatory
    ... Bipolar Outflows associated with High-Mass Young Stars are spectacular structures in the near infrared: massive eruptions of molecules accompany the star formation process. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/research/outflows.html -- 5.0 Кб -- 08.03.2013
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    8. Armagh Observatory
    ... Star Formation and Magnetohydrodynamics: one begins with clouds of molecules and dust....... one generates jets, shocks, turbulence, disks and protostars........... and one ends up with stars and planets. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/research/res-sf.html -- 5.2 Кб -- 08.03.2013
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    9. M.D. Smith, Research Astronomer
    ... spectra display emission lines from excited molecules of hydrogen which can be ... prompted Rosen and Smith to simulate fast shocks in which molecules are destroyed ... to be possible because the reformation of molecules in the post-shock cooling flow ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep2003/node62.html -- 10.8 Кб -- 19.05.2004
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    10. Spinning Star Formation
    ... Stars are born within stellar wombs: giant clouds of molecules and dust. ... This gas is moving at Mach 500, and the molecules survive. ... The molecules we observe are like beads which thread the wire, forced to move in ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/press/Spinning-Star-Formation.html -- 9.2 Кб -- 19.09.2003
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