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    91. ATNF Colloquium
    ... Planck has mapped the dust polarized emission at millimetre wavelengths over the ... we are able to image the dust polarization from the diffuse interstellar medium to ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=1284 -- 26.9 Кб -- 12.04.2016
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    92. Conclusions
    ... Cross QSO is not due to synchrotron, but can be fit with a dust-reprocessing model ... might reveal the transition from the dust emission region to the optical emission ... of a simple blackbody disk since the dust emission cuts off just above the ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/18_2/agol/paper/node6.html -- 50.3 Кб -- 08.04.2016
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    93. PhD Thesis (summary)
    ... Phillips (1993) found a bipolar outflow structure in Halpha with a similar opening angle as the dust cone (possible dust filaments in the southwestern part would be hidden by the emission in the disk). ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/ngc1808/phd_thesis.html -- 11.9 Кб -- 23.12.2007
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    94. Distribution and Kinematics of the HI in NGC 5266
    ... dust-lane and polar-ring galaxies where HI is been observed, it lies in the same plane as the dust lane or ring, the presence ... dust lane and is quite abrupt, though there is evidence for a small amount of gas ``connecting'' the outer region of the ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_1/morganti/paper/node2.html -- 57.9 Кб -- 08.04.2016
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    95. High-Latitude Clouds
    ... Preliminary results suggest that, in general, the dust in HLCs has optical properties not unlike dust observed in the Galactic plane. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/15_1/larson/paper/node1.html -- 52.0 Кб -- 08.04.2016
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    96. ATNF Science Highlights 2014
    ... The synchrotron/dust-subtracted images and the spectral energy distribution indicate additional emission beside the main synchrotron component (alpha = -0.73) and the thermal component originating from dust grains at T~22 K. Results from both the ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/highlights/2014/ -- 44.0 Кб -- 10.04.2016
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    97. http://www.atnf.csiro.au/_Mail_Archives/mmwkshp/att-0035/01-speakers2.txt
    ... AGN emission 14:55-15:15 Michael Drinkwater Dust in red quasars 15:10-15:40 ... Smith (or one of his students/postdocs) Dust and Ices in Bipolar Outflows 15:35-16 ... Robert Smith, r-smith@adfa.edu.au, Dust and ices in clouds and bipolar outflows ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/_Mail_Archives/mmwkshp/att-0035/01-speakers2.txt -- 5.8 Кб -- 17.10.2001
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    98. Theoretical expectation
    ... QSO-galaxy correlations: lensing or dust? . Scott M. Croom, PASA, 18 (2), in press. ... cross-correlation signal is that dust associated with the foreground galaxies causes ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/18_2/croom/paper/node2.html -- 60.1 Кб -- 08.04.2016
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    99. Introduction
    ... However, negative correlations require inter-galactic dust associated with the foreground lenses, making a dust explanation appear rather contrived. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/18_2/croom/paper/node1.html -- 54.3 Кб -- 08.04.2016
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    100. Conclusions
    ... We note that the dust-charge fluctuations as well as the dynamics of the dust charging process can lead to the appearance of an imaginary part in the dispersion equation (Tsytovich and Havnes 1993), leading to a damping of the wave in addition to the ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_2/cramer/paper/node5.html -- 51.3 Кб -- 08.04.2016
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