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- W3200427557 abstract "ABSTRACT Deeply embedded protostars are actively fed from their surrounding envelopes through their protostellar disc. The physical structure of such early discs might be different from that of more evolved sources due to the active accretion. We present 1.3 and 3 mm ALMA continuum observations at resolutions of 6.5 and 12 au, respectively, towards the Class 0 source IRAS 16293−2422 B. The resolved brightness temperatures appear remarkably high, with Tb > 100 K within ∼30 au and Tb peak over 400 K at 3 mm. Both wavelengths show a lopsided emission with a spectral index reaching values less than 2 in the central ∼20 au region. We compare these observations with a series of radiative transfer calculations and synthetic observations of magnetohydrodynamic and radiation hydrodynamic protostellar disc models formed after the collapse of a dense core. Based on our results, we argue that the gas kinematics within the disc may play a more significant role in heating the disc than the protostellar radiation. In particular, our radiation hydrodynamic simulation of disc formation, including heating sources associated with gravitational instabilities, is able to generate the temperatures necessary to explain the high fluxes observed in IRAS 16293B. Besides, the low spectral index values are naturally reproduced by the high optical depth and high inner temperatures of the protostellar disc models. The high temperatures in IRAS 16293B imply that volatile species are mostly in the gas phase, suggesting that a self-gravitating disc could be at the origin of a hot corino." @default.
- W3200427557 created "2021-09-27" @default.
- W3200427557 creator A5005518679 @default.
- W3200427557 creator A5017487448 @default.
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- W3200427557 creator A5070116789 @default.
- W3200427557 creator A5072625482 @default.
- W3200427557 creator A5090718980 @default.
- W3200427557 date "2021-09-20" @default.
- W3200427557 modified "2023-10-18" @default.
- W3200427557 title "The young protostellar disc in IRAS 16293−2422 B is hot and shows signatures of gravitational instability" @default.
- W3200427557 cites W1520458560 @default.
- W3200427557 cites W1639285581 @default.
- W3200427557 cites W1840952669 @default.
- W3200427557 cites W1965372241 @default.
- W3200427557 cites W1969206086 @default.
- W3200427557 cites W1977430478 @default.
- W3200427557 cites W1983270357 @default.
- W3200427557 cites W1986202073 @default.
- W3200427557 cites W1998745722 @default.
- W3200427557 cites W2006869439 @default.
- W3200427557 cites W2007993160 @default.
- W3200427557 cites W2009836081 @default.
- W3200427557 cites W2014620781 @default.
- W3200427557 cites W2017322129 @default.
- W3200427557 cites W2021347355 @default.
- W3200427557 cites W2031218180 @default.
- W3200427557 cites W2031968292 @default.
- W3200427557 cites W2033697868 @default.
- W3200427557 cites W2034608771 @default.
- W3200427557 cites W2035547408 @default.
- W3200427557 cites W2041579602 @default.
- W3200427557 cites W2042176389 @default.
- W3200427557 cites W2042484924 @default.
- W3200427557 cites W2042937985 @default.
- W3200427557 cites W2044105167 @default.
- W3200427557 cites W2081688115 @default.
- W3200427557 cites W2084926137 @default.
- W3200427557 cites W2095705361 @default.
- W3200427557 cites W2095820618 @default.
- W3200427557 cites W2098834320 @default.
- W3200427557 cites W2099559854 @default.
- W3200427557 cites W2129495060 @default.
- W3200427557 cites W2130736142 @default.
- W3200427557 cites W2143416500 @default.
- W3200427557 cites W2163613589 @default.
- W3200427557 cites W2168324082 @default.
- W3200427557 cites W2188467324 @default.
- W3200427557 cites W2203831943 @default.
- W3200427557 cites W2231411390 @default.
- W3200427557 cites W2296212688 @default.
- W3200427557 cites W2534368935 @default.
- W3200427557 cites W2620668206 @default.
- W3200427557 cites W2723569213 @default.
- W3200427557 cites W2734981119 @default.
- W3200427557 cites W2741780642 @default.
- W3200427557 cites W2757878606 @default.
- W3200427557 cites W2787515915 @default.
- W3200427557 cites W2789665953 @default.
- W3200427557 cites W2799056805 @default.
- W3200427557 cites W2888280926 @default.
- W3200427557 cites W2889156951 @default.
- W3200427557 cites W2896417422 @default.
- W3200427557 cites W2898319592 @default.
- W3200427557 cites W2898693397 @default.
- W3200427557 cites W2921982054 @default.
- W3200427557 cites W2953974790 @default.
- W3200427557 cites W2962797670 @default.
- W3200427557 cites W2963013492 @default.
- W3200427557 cites W2964562192 @default.
- W3200427557 cites W3000663721 @default.
- W3200427557 cites W3033111100 @default.
- W3200427557 cites W3035220361 @default.
- W3200427557 cites W3041409567 @default.
- W3200427557 cites W3043157458 @default.
- W3200427557 cites W3043379905 @default.
- W3200427557 cites W3077044787 @default.
- W3200427557 cites W3091806620 @default.
- W3200427557 cites W3092353545 @default.
- W3200427557 cites W3092991002 @default.
- W3200427557 cites W3097998914 @default.
- W3200427557 cites W3098760510 @default.
- W3200427557 cites W3098805460 @default.
- W3200427557 cites W3098920994 @default.
- W3200427557 cites W3099065891 @default.
- W3200427557 cites W3099078105 @default.
- W3200427557 cites W3099783294 @default.
- W3200427557 cites W3099821900 @default.
- W3200427557 cites W3099932582 @default.
- W3200427557 cites W3100423345 @default.
- W3200427557 cites W3100753209 @default.
- W3200427557 cites W3100792383 @default.
- W3200427557 cites W3101193570 @default.
- W3200427557 cites W3101217625 @default.
- W3200427557 cites W3101359137 @default.
- W3200427557 cites W3101525322 @default.
- W3200427557 cites W3103103352 @default.