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    41. Grain_growth_southernproroplanetarydisks
    ... Many young stars are surrounded by disks of gas and dust which are a natural by ... dust emission by 10 - 30 million years, but again cannot distinguish between a ... suggest the presence of mm-sized dust aggregates and hence grain growth in the disks ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/newsletter/jun06/Grain_growth.htm -- 13.5 Кб -- 23.01.2013
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    42. The Peculiar Spiral Galaxy NGC 1808
    ... In the northeastern part of the disk, where prominent dust filaments seem to emerge from the nuclear region, we find a velocity anomaly which indicates outflow of HI gas into the halo of the galaxy. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/ngc1808/n1808_hi.html -- 3.8 Кб -- 23.12.2007
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    43. ATNF Publications 2002
    ... OOSTERLOO, T.A., MORGANTI, R., SADLER, E.M.,VERGANI, D. & CALDWELL, N. "Extended H I disks in dust lane elliptical galaxies". ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/newsletter/jun02/ATnewsJun.htm -- 58.5 Кб -- 28.02.2014
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    44. Conclusions
    ... The optical/UV SED must be flatter than the prediction of a simple blackbody disk since the dust emission cuts off just above the sublimation temperature, and thus does not modify the optical spectrum. ...
    [ 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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    45. http://www.atnf.csiro.au/lists/historical/mmwkshp/att-0035/speakers2.txt
    ... Disks 14:35-14:55 Warrick Lawson Evolution of Pre-Main Sequence Stars 14:55-15:15 John Storey The IR connection 15:15-15:35 ... smaddison@swin.edu.au, Modeling Protostellar Disks Robert Smith, r-smith@adfa.edu.au, Dust and ices in clouds and bipolar ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/lists/historical/mmwkshp/att-0035/speakers2.txt -- 5.8 Кб -- 20.06.2013
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    46. http://www.atnf.csiro.au/_Mail_Archives/mmwkshp/att-0035/01-speakers2.txt
    ... Disks 14:35-14:55 Warrick Lawson Evolution of Pre-Main Sequence Stars 14:55-15:15 John Storey The IR connection 15:15-15:35 ... smaddison@swin.edu.au, Modeling Protostellar Disks Robert Smith, r-smith@adfa.edu.au, Dust and ices in clouds and bipolar ...
    [ 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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    47. http://www.atnf.csiro.au/the_atnf/annual_reports/2002/17189_p65-100.pdf
    ... 2002). Appendices OOSTERLOO, T.A., MORGANTI, R., SADLER, E.M.,VERGANI, D. & CALDWELL, N. "Extended HI disks in dust lane elliptical g alaxies". ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/the_atnf/annual_reports/2002/17189_p65-100.pdf -- 752.5 Кб -- 14.07.2003
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    48. http://www.atnf.csiro.au/pasa/15_3/masci/paper.pdf
    ... For simplicity, we assume that the dust is associated with a cylindrical face-on disk with uniform dust mass density. ... modelled these effects by assuming that dust in each galaxy was distributed as an exponential disk with scale radius r0 30 kpc ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/pasa/15_3/masci/paper.pdf -- 160.0 Кб -- 06.11.1998
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    49. Galaxy Lunch - Dave Lommen speaking on "Probing the first steps of planet
    ... The dust grains in the disks have to grow from submicron to kilometre sizes within a few million years, and the largerst grains that can be observed directly are of about centimetre sizes. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=839 -- 27.0 Кб -- 01.03.2014
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    50. Observational Program
    ... velocity distribution through the dust lane all along the disk, and with a spectral ... dust, it is also much better than the usual optical photometry when used to compare ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/14_2/bureau/paper/node3.html -- 62.6 Кб -- 08.04.2016
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