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    1. http://www.mrao.cam.ac.uk/~eic22/Papers/gbs.pdf
    ... is that it may be the result of a high-velocity cloud impacting the Galactic plane (Comeron & Torra 1992, 1994; Guillout et al ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~eic22/Papers/gbs.pdf -- 953.2 Кб -- 11.06.2009
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    2. http://www.mrao.cam.ac.uk/~rachael/compphys/CompPhys2.pdf
    ... Having found that a collision occurs we can take an appropriate action, for example (i) merger of the clouds for a slow collision; (ii) dissipation for a normal collision; (iii) break up of the clouds for a high-velocity collision. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~rachael/compphys/CompPhys2.pdf -- 866.4 Кб -- 22.10.2007
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    3. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/VBourrier.pdf
    ... carried away to high altitudes heavy species at high altitude: neutral magnesium ... high velocity, in the EXOSPHERE MgI line absorption signature : 8.8% ± 2.1% in [-60 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/VBourrier.pdf -- 1381.2 Кб -- 17.04.2014
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    4. http://www.mrao.cam.ac.uk/~krause/mk.nam-2005.pdf
    ... The observations · High redshift radio galaxies show huge emission line haloes ·The ... yes some, but some present in highest resolution spectroscopy (Wilman et al ... 2004) ·Normal narrow line clouds in ionisation cone: no, wrong kinematics ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~krause/mk.nam-2005.pdf -- 2517.6 Кб -- 04.04.2005
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    5. Scaling relations for molecular gas in the Large Magellanic Cloud
    ... clouds obey the same linewidth-size relation, (2) Virial mass-luminosity and ... higher photodissociation rates and is expected to lead to smaller and more clumpy ... clouds in the Galaxy has resulted in a number of scaling relations between global ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/heikkilae/heikkilae.html -- 14.3 Кб -- 08.12.2003
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    6. http://www.mrao.cam.ac.uk/yerac/heikkilae/heikkilae.ps
    ... Cloud By A r t o H e i kk i l Ёa e­mail: arto@oso.chalmers.se Onsala Space ... clouds obey the same linewidth­size relation, (2) Virial mass­luminosity and ... higher photodissociation rates and is expected to lead to smaller and more clumpy ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/yerac/heikkilae/heikkilae.ps -- 286.8 Кб -- 22.02.1995
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    7. High resolution studies of protostellar condensations in NGC 2024
    ... We present high resolution ( ) studies of the 3 mm dust continuum and line emission from protostellar condensations in one of the Orion B molecular cloud cores, located southwards from the ionization front of the NGC 2024 HII region. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/wiesemeyer/wiesemeyer.html -- 25.3 Кб -- 08.12.2003
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    8. Research
    ... Quasar driven outflow (high velocity gas traced by the [OIII]5007 line, white contours) quenching star formation (traced by Halpha emission, color) in a galaxy at z=2.4 ( Cano-Diaz, Maiolino et al. ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~rm665/research.html -- 35.9 Кб -- 10.03.2016
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    9. An expanding plasmon model for the radio outbursts of Cir X-1
    ... LSI , Cir X-1, etc., exhibit highly variable bursting radio emission interpreted as ... well known because the location in a highly obscured region, where three faint stars ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/garcia/garcia.html -- 13.7 Кб -- 08.12.2003
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    10. Molecular oxygen in interstellar clouds
    ... as well as possible molecular clouds which should have high intensity in this line ... molecular clouds models: represents the visual extinction througout the whole cloud ...
    [ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/yerac/marechal/marechal.html -- 17.0 Кб -- 08.12.2003
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