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    81. Armagh Observatory
    ... to show that hot gas can be ejected in three forms: jets, bubbles and clouds ... I have confirmed that Molecular Jets do indeed generate the structures observed ... hydrocode to follow the molecular-atomic transitions of hydrogen was developed with ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/research/highlights1.html -- 7.1 Кб -- 30.06.2010
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    82. Refereed Journal Publications, 1998
    ... M.D. , 1998, ``Kinetic energy decay rates of supersonic and super-Alfv?nic turbulence in star-forming clouds'', Phys. Rev. Lett ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/annrep/annrep98/node19.html -- 12.6 Кб -- 14.12.1999
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    83. http://star.arm.ac.uk/preprints/402.ps
    ... We combine molecular spectroscopic data from the submillimeter to the near infrared ... bow shock geometry can simultaneously explain all the molecular excitations ... Subject headings: Shock waves { Molecular processes { ISM: jets and out ows { ISM ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/preprints/402.ps -- 916.2 Кб -- 17.09.2003
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    84. http://star.arm.ac.uk/~csj/papers/reviews/2002_rcrb.ps
    ... fading is caused by the formation of sooty dust clouds above the surface of the star ... The fades are caused by enormous clouds of dust which cover a large part of the star ... Why the dust clouds form is harder to understand. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/papers/reviews/2002_rcrb.ps -- 214.0 Кб -- 26.06.2006
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    85. http://star.arm.ac.uk/iaj/online/v25n1p1.ps
    ... the clouds giving rise to the maser features is spherical, and that the clouds are ... 17 clouds containing multiple peaks is 60% larger than that of single peaked clouds ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/iaj/online/v25n1p1.ps -- 2313.4 Кб -- 09.01.1998
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    86. http://star.arm.ac.uk/~csj/papers/conference/2002_ATMOS_2.ps
    ... structure and chemistry of hot molecular cores,  shock chemistry associated with ... for the submillimeter will enable the 3-D exploration of interstellar clouds ... 4 Je ery 4.1. Atomic and Molecular Databases. ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/papers/conference/2002_ATMOS_2.ps -- 82.0 Кб -- 15.08.2002
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    87. http://star.arm.ac.uk/~csj/papers/conference/opt_sak.ps
    ... 23/12/2000; 20:38; p.13 14 and very low surface gravity together with an unusually carbon­rich chemistry and forests of molecular lines creates a substantial demand for molecular data and new methods to include these in spectral syn­ thesis calculations ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/papers/conference/opt_sak.ps -- 775.3 Кб -- 02.02.2001
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    88. http://star.arm.ac.uk/nibulletin/2010/Feb10.html
    ... is the most powerful telescope for observing the cool Universe вАФ molecular gas and dust as well as the relic radiation of the ... The Cassini spacecraft flew through icy clouds created by ice volcanoes detecting negatively charged water molecules. ...
    [ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/nibulletin/2010/Feb10.html -- 16.8 Кб -- 10.02.2010
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    89. http://star.arm.ac.uk/~ambn/UU_Aur.ps
    ... observed sub­mm excess: contribution of molecular lines, free­free emission, or mass ... 0:05 Їm will be destroyed by hydro­ genation and chemical sputtering in dense clouds ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~ambn/UU_Aur.ps -- 740.9 Кб -- 19.11.1996
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    90. http://star.arm.ac.uk/~csj/papers/newsletter/ccp7n21_jeffery1.ps
    ... R CrB) and those with strong CN and C 2 molecular bands (cf. S Aps). ... due to an `eclipse' of the photosphere by dense clouds of carbon­rich dust ­ or soot ... concern the composition of the dust (molecular or graphitic), the ejection mechanism ...
    [ Текст ]  Ссылки http://star.arm.ac.uk/~csj/papers/newsletter/ccp7n21_jeffery1.ps -- 137.5 Кб -- 30.10.2001
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