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    1. http://www.atnf.csiro.au/research/Astro2010/talks/liffman.pdf
    ... Transport of Processed Material in Circumstellar Disks The dust in the ISM has an ... Inner disk dust ~ 90% crystalline silicate. ... Outer disk dust ~40% crystalline silicate The dust in inner disks is more processed. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/liffman.pdf -- 2807.2 Кб -- 16.06.2010
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    2. http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch7.pdf
    ... This 'dust' disk is defined by the the density of the dust or optical depth which is ... NGC 891 with the same scale length for the dust disk as the H disk (hg = hd = 5 kpc ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch7.pdf -- 143.6 Кб -- 21.10.2013
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    3. ATNF Science Highlights 2002
    ... stars exhibit emission from circumstellar dust disks with properties similar to the ... dust continuum and HCO + ( J =1-0) line emission at 89 GHz (3.4 mm) from two young ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/highlights/2002/wilner/wilner.html -- 52.0 Кб -- 08.04.2016
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    4. Programme - Abstract
    ... about half of the mid-IR emission has a size of 0.6 0.2 pc (FWHM) and is consistent with an inclined, disk-like dust structure ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/cena/programme_show_abstract_bur.php -- 4.6 Кб -- 02.10.2012
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    5. Programme - Abstract
    ... Since our results showed kinematics of the dust warped disk, we will discuss kinematics and physical properties in the dust lane of Centaurus A. go back . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/cena/programme_show_abstract_oku.php -- 3.9 Кб -- 02.10.2012
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    6. http://www.atnf.csiro.au/research/masermeeting/web_papers/305_DeBuizer.pdf
    ... or extended MIR may generally come from outflows, not disks MIR dust emission SiO Outflow De Buizer, Redman, Feldman, Longmore ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/305_DeBuizer.pdf -- 1452.2 Кб -- 26.03.2007
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    7. http://www.atnf.csiro.au/research/cena/documents/presentations/israel.pdf
    ... Recent merger elliptical and small spiral Dark band is thin tilted disk dust and gas Precessing jets from SMBH 5.5 x 107 MO Submilliarcsec nucleus AV = 1216 mag Ongoing Accretion? ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/cena/documents/presentations/israel.pdf -- 2308.3 Кб -- 16.07.2009
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    8. http://www.atnf.csiro.au/people/Amy.Kimball/Publications/agol_et_al_2009.pdf
    ... dusty torus is heated by radiation from the accretion disk, but dust cannot exist at temperatures above about 1500 K, causing a ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Amy.Kimball/Publications/agol_et_al_2009.pdf -- 300.6 Кб -- 02.10.2013
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    9. http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch1.pdf
    ... This is because the dust disks in these small galaxies are much more puffed up compared to the ones in their massive (vrot ... They used the same double exponential to fit the extinction in the disk, thus in a manner of speaking the dust disk. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/people/Peter.Kamphuis/Thesis/ch1.pdf -- 1166.3 Кб -- 21.10.2013
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    10. http://www.atnf.csiro.au/research/conferences/2014/ThePeripheryOfDisks/POD_Abstracts.pdf
    ... one tracer of star-formation driven outflows from galaxy disks: extraplanar dust ... Observations of dust in the interstellar thick disks of spiral galaxies have ... 110 galaxies we detect the emission of a dust disk out to twice the optical radius ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/conferences/2014/ThePeripheryOfDisks/POD_Abstracts.pdf -- 124.8 Кб -- 02.11.2014
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