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    1. http://www.mso.anu.edu.au/seminars/abstracts/20151106-1400.html
    ... Similar WD-WD collisions, occurring in the thick disk, ultimately supply much of the 511 keV radiation emission extending along the Galactic plane.. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151106-1400.html -- 4.7 Кб -- 10.04.2016
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    2. Julie Banfield | Astronomer
    ... where galaxies undergo high-speed collisions, ram pressure stripping and tidal ... falling into the cluster through radio observations of active galactic nuclei (AGN ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~julie/ -- 11.6 Кб -- 09.04.2016
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    3. Blue Straggler Stars
    ... Globular clusters are located in galactic halos, of which the Milky Way may have ... there are more stars per unit volume, collisions and close-encounters are far more ... What about Galactic extinction? ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~jerjen/researchprojects/bluestraggler/bluestraggler.html -- 9.1 Кб -- 02.10.2012
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    4. http://www.mso.anu.edu.au/~fbriggs/LOFAR_SciApp_1.0.pdf
    ... the relativistic electrons causing the extended emission (see reviews by Jaffe 1992, Feretti & Giovannini 1995), involving (i) particle collisions (Vestrand 1982), (ii) galactic wakes (Roland 1981), (iii) intracluster turbulence and shocks (Harris et al ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~fbriggs/LOFAR_SciApp_1.0.pdf -- 1914.3 Кб -- 17.04.2003
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    5. http://www.mso.anu.edu.au/~brian/A3002/lect11.pdf
    ... self-consistent solution parameters Better Modeling, especially at H I collisions low Z Two Recent Results Source Izotov et al ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~brian/A3002/lect11.pdf -- 1254.2 Кб -- 23.10.2006
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    6. RSAA Annual Report 1998
    ... The existence of these latter stars indicates that And II, like all the Galactic dSphs, does contain a population as old as the globular clusters of the Galactic halo. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1998/07_research.html -- 53.8 Кб -- 02.10.2012
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    7. http://www.mso.anu.edu.au/~bessell/Beauty.ps
    ... the LMC and SMC and are mapping the Galactic Plane for comparison with the Molonglo ... with their Molonglo Radio Surveys of the galactic plane (Green et al. 1999; http ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~bessell/Beauty.ps -- 139.3 Кб -- 28.01.2004
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    8. http://www.mso.anu.edu.au/pfrancis/comets/comets.pdf
    ... The comets are weakly concentrated at intermediate galactic latitudes (Fig 5), consistent with the galactic tide playing a ma jor part in making them observable (Matese & Whitmire 1996). ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/comets/comets.pdf -- 1827.0 Кб -- 06.09.2005
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    9. http://www.mso.anu.edu.au/~geoff/HEA/5_Compton_Scattering_I.pdf
    ... the collision are: = h = Initial photon energy 1 = h 1 = Final photon energy m e c 2 = Initial electron energy E = Final electron energy = Angle of deflection of photon High Energy Astrophysics: Compton Scattering I 8/59 Treatment of collision using 4 ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/5_Compton_Scattering_I.pdf -- 105.7 Кб -- 27.05.2003
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    10. http://www.mso.anu.edu.au/~charley/papers/MinierLineweaver2006.pdf
    ... 1979), late M-type stars (Dickinson 1976) and Active Galactic Nuclei (Claussen et al ... the impact on Jupiter induced by the Shoemaker-Levy comet collision (Bjoraker et al ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/MinierLineweaver2006.pdf -- 75.8 Кб -- 28.02.2007
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