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    1. Summary
    ... by assuming that the optically unseen secondary is a disk of gas and dust which is in centrifugal balance in the radial ... demonstrates that the Aurig? disk is well-modeled by a gas/dust disk with a scale height at its outer edge that is 3% of the ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/node92.html -- 20.3 Кб -- 01.10.2012
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    2. SAO Summer Intern Program Projects, 2012
    ... are any infrared lines that might help to categorize the object; (2) any faint dust features that might help to characterize the dust disk around the throat of the nucleus; (3) model the mid-IR spectra energy shape more precisely by combining the spectral ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2012/projects12.html -- 20.9 Кб -- 27.02.2014
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    3. http://hea-www.harvard.edu/~kim/pap/2015_Scaling.pdf
    ... 2009; Lauer 2012). The morphological type could be misclassified due to hidden disks or dust obscuration. ... 13. Dust features: D (dusty disk), F (dusty filament), B (blue nucleus) and BR (blue ring) from Krajnovi, D. et al. (2011). 14. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2015_Scaling.pdf -- 688.7 Кб -- 15.10.2015
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    4. http://hea-www.harvard.edu/~bradw/cv/papers/whiteGenX.pdf
    ... In each case, the overall disk structure, dust and molecular composition wil l have been measured using the Spitzer, Herschel, JWST, and ALMA telescopes. ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~bradw/cv/papers/whiteGenX.pdf -- 434.2 Кб -- 08.10.2009
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    5. Intern Directory
    ... Brant Robertson . Churchill scholar, Cambridge (2005); PhD Caltech 2010; geologist for Shell . Stellar dust disks . Anandi Salinas . UT Austin . ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~jcm/intern/intern.html -- 74.8 Кб -- 10.04.2016
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    6. http://hea-www.harvard.edu/QEDT/Papers/color-color.ps
    ... emission model and non­thermal power law or dust, irradiation of the disk surface ... the size of dust grains, the size of the dust region, the disk inclination angle ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/QEDT/Papers/color-color.ps -- 787.9 Кб -- 04.04.1995
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    7. http://hea-www.harvard.edu/AstroStat/Stat310_1314/bc_20140408.pdf
    ... temperature is below 1000 K and allows for dust formation Ouflow is cased by radiation pressure acting on dust grains Far from the disk the dusty clouds are irradiated and dust evaporates Dustless material looses support against gravity and falls back ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_1314/bc_20140408.pdf -- 927.1 Кб -- 07.04.2014
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    8. http://hea-www.harvard.edu/~kim/pap/2012_N4278_Silvia.pdf
    ... in a rotating, inner disk, and of the warm dust emission detected with Spitzer ... the nucleus sitting in a small unobscured hole at the center of a thin dust disk ... that the inner dust resides in a thin, moderately inclined disk, whose major axis ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2012_N4278_Silvia.pdf -- 2396.2 Кб -- 02.05.2013
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    9. Disk Expansion and Absorption Line Profiles
    ... in the above scalings, or directly from the realization that when pressure support is removed, gas molecules and dust travel on free-fall orbits, which must intersect the disk midplane exactly twice each orbit and thus require 1/4 orbit from peak to node ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/node91.html -- 14.2 Кб -- 01.10.2012
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    10. Vertical Structure of the Secondary: Hydrostatic Model
    ... The scale height of the disk is assumed to be proportional to the distance from the ... The opacity of the gas/dust mixture, (in units of cm /g), is a function of ... optical depth which we observe through the disk at a given point on the projected ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/node89.html -- 10.7 Кб -- 01.10.2012
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