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• W3099879872 endingPage "100" @default.
• W3099879872 startingPage "100" @default.
• W3099879872 abstract "Protostellar systems, ranging from low-luminosity T Tauri and Herbig Ae stars to high-luminosity Herbig Be stars, exhibit a near-infrared (NIR) excess in their spectra that is dominated by a bump in the monochromatic luminosity with a peak near 3 microns. The bump can be approximated by a thermal emission component of temperature 1500 K that is of the order of the sublimation temperature of interstellar dust grains. In the currently popular puffed up rim scenario, the bump represents stellar radiation that propagates through the optically thin inner region of the surrounding accretion disk and is absorbed and reemitted by the dust that resides just beyond the dust sublimation radius, Rsub. However, this model cannot account for the strongest bumps measured in these sources, and it predicts a large secondary bounce in the interferometric visibility curve that is not observed. In this paper we present an alternative interpretation, which attributes the bump to reemission of stellar radiation by dust that is uplifted from the disk by a centrifugally driven wind. Winds of this type are a leading candidate for the origin of the strong outflows associated with protostars, and there is observational evidence for disk winds originating on scales ~Rsub. Using a newly constructed Monte Carlo radiative transfer code, we show that this model can account for the NIR excess emission even in bright Herbig Ae stars such as AB Auriga and MWC 275, and that it successfully reproduces the basic features of the visibilities measured in these protostars. We argue that a robust dusty outflow in these sources could be self-limiting to a relatively narrow launching region between Rsub and 2Rsub. Finally, we suggest that our model could also naturally account for the NIR and scattered-light variability exhibited by a source like MWC 275, which may be triggered by the uplifting of dust clouds from the disk." @default.
• W3099879872 created "2020-11-23" @default.
• W3099879872 creator A5047280575 @default.
• W3099879872 creator A5078872301 @default.
• W3099879872 date "2012-10-05" @default.
• W3099879872 modified "2023-10-03" @default.
• W3099879872 title "A DISK-WIND MODEL FOR THE NEAR-INFRARED EXCESS EMISSION IN PROTOSTARS" @default.
• W3099879872 cites W1617577911 @default.
• W3099879872 cites W1622101081 @default.
• W3099879872 cites W1967407002 @default.
• W3099879872 cites W1967675813 @default.
• W3099879872 cites W1968443772 @default.
• W3099879872 cites W1972551044 @default.
• W3099879872 cites W1972594415 @default.
• W3099879872 cites W1975107251 @default.
• W3099879872 cites W1977727133 @default.
• W3099879872 cites W1980100166 @default.
• W3099879872 cites W1980288144 @default.
• W3099879872 cites W1985967817 @default.
• W3099879872 cites W1989803327 @default.
• W3099879872 cites W2000369716 @default.
• W3099879872 cites W2000417483 @default.
• W3099879872 cites W2005018826 @default.
• W3099879872 cites W2005467021 @default.
• W3099879872 cites W2005684104 @default.
• W3099879872 cites W2008132488 @default.
• W3099879872 cites W2012630673 @default.
• W3099879872 cites W2013032016 @default.
• W3099879872 cites W2017464195 @default.
• W3099879872 cites W2019274761 @default.
• W3099879872 cites W2019754078 @default.
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• W3099879872 cites W2027490520 @default.
• W3099879872 cites W2030251810 @default.
• W3099879872 cites W2031220985 @default.
• W3099879872 cites W2033756463 @default.
• W3099879872 cites W2034608771 @default.
• W3099879872 cites W2035693616 @default.
• W3099879872 cites W2047754542 @default.
• W3099879872 cites W2048316219 @default.
• W3099879872 cites W2048587018 @default.
• W3099879872 cites W2054257845 @default.
• W3099879872 cites W2055069090 @default.
• W3099879872 cites W2056508188 @default.
• W3099879872 cites W2062666861 @default.
• W3099879872 cites W2064258363 @default.
• W3099879872 cites W2064977824 @default.
• W3099879872 cites W2065864905 @default.
• W3099879872 cites W2084604096 @default.
• W3099879872 cites W2086180078 @default.
• W3099879872 cites W2096570366 @default.
• W3099879872 cites W2099559854 @default.
• W3099879872 cites W2110894057 @default.
• W3099879872 cites W2115932981 @default.
• W3099879872 cites W2117821269 @default.
• W3099879872 cites W2127867276 @default.
• W3099879872 cites W2132564213 @default.
• W3099879872 cites W2137346297 @default.
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• W3099879872 cites W2156621121 @default.
• W3099879872 cites W2161357664 @default.
• W3099879872 cites W2161791806 @default.
• W3099879872 cites W2163780026 @default.
• W3099879872 cites W2168426271 @default.
• W3099879872 cites W2171291743 @default.
• W3099879872 cites W3099199047 @default.
• W3099879872 cites W3100581532 @default.
• W3099879872 cites W3101295379 @default.
• W3099879872 cites W3101646687 @default.
• W3099879872 cites W3103071107 @default.
• W3099879872 cites W3103376136 @default.
• W3099879872 cites W3104329102 @default.
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• W3099879872 cites W3105988269 @default.
• W3099879872 cites W4247735440 @default.
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• W3099879872 doi "https://doi.org/10.1088/0004-637x/758/2/100" @default.
• W3099879872 hasPublicationYear "2012" @default.
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