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    41. http://hea-www.harvard.edu/~garcia/apj.555.477.ps
    ... that is caused by an accretion disk with a large inner disk radius : The second is a ... disk spectrum shown in Figure 3 is speciпed by two parameters : (1) the temperature ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~garcia/apj.555.477.ps -- 1112.1 Кб -- 08.02.2011
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    42. http://hea-www.harvard.edu/~kim/pap/ULX_N4244.pdf
    ... a complex spectral shape; a multicolor disk model, suitable for brighter ULXs, is ... 0.3 and 10.0 keV with an absorbed power-law model and an absorbed disk blackbody ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/ULX_N4244.pdf -- 195.2 Кб -- 06.12.2010
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    43. http://hea-www.harvard.edu/QEDT/Papers/rosat_bals.ps
    ... A low dust­to­gas ratio might seem strange in an IRAS QSO where much of the far­IR luminosity is expected to be from warm dust ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/QEDT/Papers/rosat_bals.ps -- 166.6 Кб -- 11.01.1996
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    44. SAO Summer Intern Program Projects, 2014
    ... brown dwarfs that might be part of the thin disk stellar population, or the slightly puffier thick disk, or even the halo ... The coolest and faintest ones ought to be detectable in at least the thin disk if not the thick disk also. ...
    [ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/REU/2014/projects14.html -- 25.2 Кб -- 10.04.2016
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    45. http://hea-www.harvard.edu/~pgreen/Papers/SDSS1254.pdf
    ... quasar accretion disks are reasonably well aligned with their galactic host disks,11 ... initial equilibrium disk models are constructed to be representative of disks at the ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~pgreen/Papers/SDSS1254.pdf -- 1028.8 Кб -- 02.02.2010
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    46. http://hea-www.harvard.edu/~kim/pap/Sombrero.pdf
    ... luminosity, inconsistent with efficient disk accretion, there are other properties by which the Sombrero's nucleus differs from Seyfert 1 nuclei: (1) the latter exhibit Fe K emission lines produced in the accretion disk whose strength clearly increases ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/Sombrero.pdf -- 374.3 Кб -- 06.12.2010
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    47. http://hea-www.harvard.edu/~kim/pap/2009_ChaMP_anca_apj.pdf
    ... 2002), the (dust corrected) stellar mass M (Kauffmann et al. 2003a), the Balmer decrement H/H as a proxy for dust extinction ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~kim/pap/2009_ChaMP_anca_apj.pdf -- 1675.1 Кб -- 06.12.2010
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    48. http://hea-www.harvard.edu/ChaMPlane/papers/0901-draft-maureen-lw_cv.pdf
    ... the accretion disk, the accretion stream or sometimes the white dwarf, and show Balmer emission lines from the disk or stream ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/ChaMPlane/papers/0901-draft-maureen-lw_cv.pdf -- 693.1 Кб -- 09.02.2009
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    49. http://hea-www.harvard.edu/~garcia/groot.ps
    ... by large column densities of gas and dust, obscuring the GRB afterglows (Groot et al ... forming regions where large quantities of gas and dust are present (e.g. Paczy'nski ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/~garcia/groot.ps -- 1199.2 Кб -- 08.02.2011
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    50. http://hea-www.harvard.edu/ChaMPlane/papers/0805-draft-jaesub-xray_dist.ps
    ... is derived from the Galactic stel­ lar model, which consists of the central spherical cluster, the central disk, the triaxial ellipsoidal GB and the Galactic disk (Muno et al. 2006, hereafter M06; Launhardt et al. 2002, here­ after L02; Kent et al. 1991 ...
    [ Текст ]  Ссылки http://hea-www.harvard.edu/ChaMPlane/papers/0805-draft-jaesub-xray_dist.ps -- 2015.5 Кб -- 12.06.2008
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