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    1. http://www.naic.edu/~tghosh/a1908/thesis1-final.pdf
    ... Some of the most important IRAS observations include the following: a disk of dust grains around the star Vega, six new comets, infrared cirrus (wisps of warm dust) which could be found in almost every direction of space, the core of the Milky Way, and ...
    [ Текст ]  Ссылки http://www.naic.edu/~tghosh/a1908/thesis1-final.pdf -- 2480.3 Кб -- 11.05.2007
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    2. Heiles Symposium Presentations
    ... Scientific Presentations . Diffuse, neutral gas and dust (Chair: W. Reach) . ... Warm ionized material & disk/halo interaction (Chair: R. Reynolds) . ... F. Boulanger - Properties of interstellar dust . W. Reach - Dust in the CNM/WNM . ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/~astro/heiles/Scientific_Presentations.html -- 7.2 Кб -- 23.08.2006
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    3. http://www.naic.edu/~astro/chicago2/talks/Lazio-Minding_the_Gaps.pdf
    ... 1 cm) offer unique information about planetary formation · Pebble accretion--crucial and poorly understood regime of planetary formation · Unhindered by dust obscuration Minding the Gap Imaging Protoplanetary Disks Why don't pebbles destroy each other ...
    [ Текст ]  Ссылки http://www.naic.edu/~astro/chicago2/talks/Lazio-Minding_the_Gaps.pdf -- 1775.4 Кб -- 21.08.2006
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    4. Diffuse Galactic Light in the Large Magellanic Cloud
    ... The phenomenon arises from starlight scattering off numerous dust clouds in and above the plane of the LMC's disk to form a faint, galaxy-wide reflection nebula. ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/30dor/lmc_dgl.html -- 2.4 Кб -- 09.04.2008
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    5. http://www.naic.edu/~astro/chicago2/talks/Sargent-Stars_Planets_Working_Group.pdf
    ... Major Challenges How do planets grow in circumstellar disks? Dust to pebbles to boulders How do very young stars evolve? ...
    [ Текст ]  Ссылки http://www.naic.edu/~astro/chicago2/talks/Sargent-Stars_Planets_Working_Group.pdf -- 112.9 Кб -- 21.08.2006
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    6. http://www.naic.edu/~astro/frontiers/ska_ds.pdf
    ... and the formation of stable planetary systems that include planets in habitable zones around stars: formation of massive dust and gas disks, agglomeration of planetesimals, growth of planets from the planetesimals, and a final clearing of the debris disks ...
    [ Текст ]  Ссылки http://www.naic.edu/~astro/frontiers/ska_ds.pdf -- 1616.0 Кб -- 19.12.2007
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    7. http://www.naic.edu/~newslet/no26/NAICNo26.pdf
    ... Celia SalmerСn (Univ. of Houston) worked with Carmen Pantoja (UPR) to get a picture of a spiral galaxy hidden behind the gas and dust in the disk of the Galaxy. ...
    [ Текст ]  Ссылки http://www.naic.edu/~newslet/no26/NAICNo26.pdf -- 479.0 Кб -- 14.12.1998
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    8. http://www.naic.edu/~astro/chicago2/talks/Reid-Science_with_Future_Radio_Telescopes.pdf
    ... BH Synchrotron emission from Accretion disk, Magnetic connections (BH ­ disk), Jet formation / acceleration Pulsars Estimated ...
    [ Текст ]  Ссылки http://www.naic.edu/~astro/chicago2/talks/Reid-Science_with_Future_Radio_Telescopes.pdf -- 1804.7 Кб -- 21.08.2006
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    9. http://www.naic.edu/~gibson/asph405/dry/drylab.ps.gz
    ... an infinite, plane­parallel Galactic ``atmosphere'' to find A g as a function of Galactic latitude b. This approximation has two main flaws: (1) the distribution of dust in the ISM is lumpy, not smooth, and (2) the Milky Way's disk has an outer edge ...
    [ Текст ]  Ссылки http://www.naic.edu/~gibson/asph405/dry/drylab.ps.gz -- 232.3 Кб -- 17.12.2000
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    10. I-GALFA Infrared Emission
    ... Comparisons of hydrogen gas and dust emission in other parts of the sky are available for the Perseus and MBM 53-55 molecular ...
    [ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/galfa/igalfa/gallery/iris/ -- 3.6 Кб -- 02.06.2009
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