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    11. http://www.arcetri.astro.it/~lt/projects/kona.ps.gz
    ... The dust in the disk midplane has opacity  = 0:01(=1:3mm) 1 cm 2 g 1 . ... in the near-infrared, where one is sensitive to the lack of the hottest disk dust ... it seems natural to associate at disks with dust sedimentation toward the midplane ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/projects/kona.ps.gz -- 37.4 Кб -- 11.09.2007
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    12. http://www.arcetri.astro.it/radtran/talks/lhunt.pdf
    ... Tracing Dust in Spiral Galaxies Ghent 1317 May 2007 Twodimensional bulge/disk ... are Traci virtually independent of disks. ng Dust in Spiral Galaxies Ghent 1317 May ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/radtran/talks/lhunt.pdf -- 1913.8 Кб -- 28.05.2007
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    13. NASA's Observatorium--Image Gallery: Stars
    ... Dividing the nebula in two is a dense, edge-on disk of dust and gas which appears as the thick, dark band crossing the center ... Dark clouds and bright wisps above and below the disk suggest that it is still building up from infalling dust and gas. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/StarNebula.htm -- 2.1 Кб -- 29.03.2002
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    14. http://www.arcetri.astro.it/~sbianchi/home/Simone_Bianchis_Homepage_files/curr_en.pdf
    ... 12/2009 James Clerk Maxwell Telescope, Hawaii, USA: An extended dust disk in NGC 891 ... Truncated dust disks in HI-deficient spirals, 2010, Astronomy and Astrophysics, 518 ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sbianchi/home/Simone_Bianchis_Homepage_files/curr_en.pdf -- 127.1 Кб -- 19.01.2016
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    15. http://www.arcetri.astro.it/~lt/preprints/bd_roph/bd_roph.pdf
    ... The dust in the disk midplane has opacity = 0.01(/1.3 mm)-1 cm2 g-1 (Beckwith et al. ... in the near-infrared, where one is sensitive to the lack of the hottest disk dust ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/bd_roph/bd_roph.pdf -- 1910.5 Кб -- 11.09.2007
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    16. http://www.arcetri.astro.it/~lt/preprints/uxors_vla/uxors_vla.ps.gz
    ... We describe the opacity of the dust in the disk midplane as a power­law function of ... The mass of dust in the disk is ё 1:5 \Theta 10 \Gamma4 M fi , again typical of ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/uxors_vla/uxors_vla.ps.gz -- 167.2 Кб -- 11.09.2007
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    17. http://www.arcetri.astro.it/~lt/preprints/hae_dust/natta.ps.gz
    ... the observations, determining the properties of dust in disks surrounding pre-main ... on radius ( / R p ), the properties of dust on the disk surface and in the midplane ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/hae_dust/natta.ps.gz -- 92.9 Кб -- 11.09.2007
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    18. NASA's Observatorium--Image Gallery: Stars
    ... The apparent "pinching" of this nebula close to the binary suggests that a ring or disk of dust and gas surrounds the two stars. Image: NASA. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/DoubleFormation.htm -- 2.0 Кб -- 29.03.2002
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    19. Dust evolution across the CO snowline in a protoplanetary disk
    ... This process is thought to occur in circumstellar disks of gas and dust around young stars on rather short timescales : infrared surveys show that the number of low mass stars with disks drops dramatically for stars older than 10 Myr, suggesting that in ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/home-english/204-scientific-news/1098-snow-alma -- 30.1 Кб -- 10.04.2016
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    20. http://www.arcetri.astro.it/~sperello/AA540_A52.pdf
    ... Such effects naturally arise if the dust disk is less extended than the Hi and ... have also clearly demonstrated that the dust disk is significantly reduced in very ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/AA540_A52.pdf -- 1370.1 Кб -- 24.07.2012
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