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    71. Galaxies Behind the Deepest Extinction Layer of the Southern Milky Way
    ... Abstract. About 25% of the optical extragalactic sky is obscured by the dust and stars of our Milky Way. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Baerbel.Koribalski/publications/deepsouth.html -- 3.0 Кб -- 23.12.2007
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    72. 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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    73. http://www.atnf.csiro.au/research/masermeeting/web_papers/307_Hill.pdf
    ... IR excellent tracer: Z Stars emit bulk of radiation at wavelengths shorter than Lymann continuum limit Z Circumstellar dust envelope absorbs radiation and re-emits in the infrared. ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/307_Hill.pdf -- 836.7 Кб -- 09.04.2007
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    74. http://www.atnf.csiro.au/research/Astro2010/talks/harvey-smith.pdf
    ... Correct each EM for extinction by interstellar dust (assume dust in front) 4. ... Dust correction assumes all dust is in front of HII region. 1 n0 [cm ] 10 14 Wednesday, 16 June 2010 Results: Derived ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/harvey-smith.pdf -- 1429.5 Кб -- 16.06.2010
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    75. On the absence of molecular absorption in high redshift millimetre-band...
    ... However, our survey makes the assumption that the reddening is associated with dust close to the emission redshift of the quasar and that the narrow millimetre component of this emission is intercepted by the compact molecular cores. ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Matthew.Whiting/papers/html_abstracts/highz_mm_absorption.html -- 4.1 Кб -- 05.02.2013
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    76. ATNF Colloquium by Prof. Richard Wielebinski
    ... em>``Warm Gas and Cold Dust in Galaxies plus Project APEX''</em><BR> . ... d dust. At sub-mm wavelengths the lines become a forest and the continuum emissi . ... on comes from warm dust. <BR> . ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/news/news.php?action=show_item&item_id=879 -- 27.3 Кб -- 01.03.2014
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    77. The IR Spectral Energy Distribution
    ... The infrared spectrum can be fit with a thin (i.e. dense) shell of dust with the temperature as a function of radius determined by reradiation of the QSO light (which may be absorbed by dust further in). ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/18_2/agol/paper/node5.html -- 50.5 Кб -- 08.04.2016
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    78. http://www.atnf.csiro.au/research/Astro2010/talks/liffman.pdf
    ... 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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    79. http://www.atnf.csiro.au/research/masermeeting/web_papers/305_DeBuizer.pdf
    ... 3-30 um) ­ Heat radiation from circumstellar dust ­ From 1000 K at 3 um to 100 K at ... of hot-warm (300-30K) thermal dust emission cm continuum detection rate towards ... come from outflows, not disks MIR dust emission SiO Outflow De Buizer, Redman ...
    [ Текст ]  Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/305_DeBuizer.pdf -- 1452.2 Кб -- 26.03.2007
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    80. QSO-galaxy cross-correlations
    ... QSO-galaxy correlations: lensing or dust? . Scott M. Croom, PASA, 18 (2), in press. ... If we consider a dust interpretation, then we see that must be a function of , but ...
    [ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pasa/18_2/croom/paper/node3.html -- 55.8 Кб -- 08.04.2016
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