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    41. http://www.mso.anu.edu.au/~charley/papers/DavisDaviesLineweaver.pdf
    ... 2. Dust-filled universe The simplest case to consider is the classic homogeneous, isotropic FRW universe filled with pressureless dust. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~charley/papers/DavisDaviesLineweaver.pdf -- 418.8 Кб -- 15.11.2009
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    42. http://www.mso.anu.edu.au/pfrancis/ObsTech/BrightnessUnits.pdf
    ... This curve is not constant, but varies with the amount of water vapour and dust atmosphere. ... Once again there are standard corrections (assuming average dust properties in the atmosphere) but to get higher precision you ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/ObsTech/BrightnessUnits.pdf -- 468.8 Кб -- 11.04.2007
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    43. RSAA Annual Report 1998
    ... Photoelectric Heating by Dust in Planetary Nebulae . ... die, they eject clouds of gas and dust which become ionised in the planetary nebula ... for the atomic processes, they have not treated the physics of the dust very well ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1998/07_research.html -- 53.8 Кб -- 02.10.2012
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    44. http://www.mso.anu.edu.au/pfrancis/roleplay/newstarform.pdf
    ... to figure out how they formed, or maybe pictures of swirls of dust in space (tiny grains of solid material floating amidst the ... Curiously, most of these stars were surrounded by spinning disks of gas and dust, about 1013 metres across. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/pfrancis/roleplay/newstarform.pdf -- 58.2 Кб -- 15.04.2004
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    45. Untitled1
    ... They showed that the properties of the dust torus are consistent with it being an accretion flow toward the nucleus, with most of the far-IR emission arising in the dust sublimation region a few light years from the nucleus itself. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1997/07_research.html -- 73.5 Кб -- 02.10.2012
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    46. http://www.mso.anu.edu.au/seminars/abstracts/20151009-1400.html
    ... We measure a mean ratio of A_{V}/A_{Ks}~ 13.50, and find a ~100% systematic offset with additional ~40% scatter in the reddening estimates from the Planck dust maps. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151009-1400.html -- 4.6 Кб -- 10.04.2016
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    47. http://www.mso.anu.edu.au/seminars/abstracts/20151022-1100.html
    ... In some cases, we observe occultations by coherent dust clumps which may be the precursors to planetesimals. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20151022-1100.html -- 5.0 Кб -- 10.04.2016
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    48. Untitled Document
    ... The NIFS is an infra-red device which will allow researchers to probe areas of the Universe which are shielded from view by cosmic dust. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~brian/press/Innovation.html -- 8.3 Кб -- 01.10.2012
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    49. Raquel Salmeron's Publications
    ... Magnetorotational instability in protoplanetary discs: The effect of dust grains . Salmeron, R., K?nigl, A. & Wardle, M. 2007. Ap.& ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~raquel/pubs.html -- 7.4 Кб -- 01.10.2012
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    50. Publications
    ... MSX sources in the LMC: Dust-enshrouded AGB stars, post-AGB stars and PN . ... MSX sources in the LMC: dust-enshrouded AGB stars and post-AGB stars . ... Monitoring of dust-enshrouded AGB stars in the LMC . Wood P.R. 1998, A , 338,592 . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~wood/Papers.html -- 5.2 Кб -- 01.10.2012
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