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    1. Twisting and shocking jets
    ... Twisting and shocking jets This is an extract of the central region of a frame in Movie 1, showing the twisting of the jet and the production of shocks. б© Copyright: Curtis Saxton, Geoff Bicknell, Ralph Sutherland and Stuart Midgley . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gallery3/index.php/theory/jets/erupt03_320_crop -- 10.3 Кб -- 28.02.2014
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    2. http://www.mso.anu.edu.au/seminars/abstracts/20150417-1420.html
    ... Anne Medling . "Shocks in SAMI Galaxies". ... properties, in particular the complexities associated with identifying shocks and some of the interesting galaxy features we ve ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150417-1420.html -- 4.0 Кб -- 10.04.2016
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    3. http://www.mso.anu.edu.au/seminars/abstracts/20150821-1400.html
    ... Elise Hampton . "Annual Thesis Presentation: The Interplay between star formation, shocks and AGN in merging galaxy systems". ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150821-1400.html -- 4.1 Кб -- 10.04.2016
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    4. http://www.mso.anu.edu.au/~geoff/AGD/Relativistic_Applications.pdf
    ... in the jets are shock waves · Two possibilities for creation of the shocks include ... shock Jet ISM Cocoon material Contact discontinuity Contact discontinuity Jet ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/AGD/Relativistic_Applications.pdf -- 222.7 Кб -- 29.08.2000
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    5. http://www.mso.anu.edu.au/seminars/abstracts/20160329-1100.html
    ... Moreover, their propagation is possibly changing the properties and evolution of the host galaxies and their environments through heating by shocks and/or mixing, and removing of gas by shocks and transfer of momentum. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20160329-1100.html -- 4.8 Кб -- 10.04.2016
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    6. Marc White - Astrophysicist - The Australian National University
    ... may be emitted by a turbulent, shock- excited mixing layer along the boundaries of ... We utilize MAPPINGS IV shock models to determine the fraction of total emission that ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~mwhite/publications.php -- 12.6 Кб -- 09.04.2016
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    7. Dopita Papers
    ... shock and precursor region is then dominated by the photoionized gas, rather than by ... shocks become supported by magnetic pressure in the photoionization / recombination ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~mad/madpubls.html -- 17.0 Кб -- 01.10.2012
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    8. http://www.mso.anu.edu.au/seminars/abstracts/20150825-1100.html
    ... I show how, by combining data analysis with detailed photoionisation and shock modelling, we are gaining a new understanding of the physics of both Seyfert and LINER galaxies. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150825-1100.html -- 4.1 Кб -- 10.04.2016
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    9. Siding Spring Survey
    ... Australian Bedout crater (Becker et al., 2004) associated with the Permian- Triassic "great dying" (although the presence of shock metamorphism has not yet been adequately demonstrated), strongly suggests that impacts by minor planets play an important ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~rmn/ -- 11.4 Кб -- 23.12.2011
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    10. http://www.mso.anu.edu.au/seminars/abstracts/20141204-1100.html
    ... made about the Bubbles: they contain giant shocks at heights of ~2 kpc above the ... These shocks reveal themselves as huge linear structures in radio polarization ... The shocks are sites for cosmic ray acceleration. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20141204-1100.html -- 5.2 Кб -- 10.04.2016
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