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• W3161502646 endingPage "164" @default.
• W3161502646 startingPage "164" @default.
• W3161502646 abstract "Abstract We aim at estimating the dust scale height of protoplanetary disks from millimeter continuum observations. First, we present a general expression of intensity of a ring in a protoplanetary disk and show that we can constrain the dust scale height by the azimuthal intensity variation. Then, we apply the presented methodology to the two distinct rings at 68 au and at 100 au of the protoplanetary disk around HD 163296. We constrain the dust scale height by comparing the high-resolution millimeter dust continuum image obtained in the Disk Substructures at High Angular Resolution Project (DSHARP) with radiative transfer simulations using RADMC-3D. We find that h d / h g > 0.84 at the inner ring and h d / h g < 0.11 at the outer ring with 3 σ uncertainties, where h d is the dust scale height and h g is the gas scale height. This indicates that the dust is flared at the inner ring and settled at the outer ring. We further constrain the ratio of the turbulence parameter α to the gas-to-dust-coupling parameter St from the derived dust scale height; α /St > 2.4 at the inner ring, and α /St < <?CDATA $1.1times {10}^{-2}$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mn>1.1</mml:mn> <mml:mo>×</mml:mo> <mml:msup> <mml:mn>10</mml:mn> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>2</mml:mn> </mml:mrow> </mml:msup> </mml:math> at the outer ring. This result shows that the turbulence is stronger or the dust is smaller at the inner ring than at the outer ring." @default.
• W3161502646 created "2021-05-24" @default.
• W3161502646 creator A5024572683 @default.
• W3161502646 creator A5037388966 @default.
• W3161502646 date "2021-05-01" @default.
• W3161502646 modified "2023-10-17" @default.
• W3161502646 title "Estimate on Dust Scale Height from the ALMA Dust Continuum Image of the HD 163296 Protoplanetary Disk" @default.
• W3161502646 cites W1977430478 @default.
• W3161502646 cites W1982757757 @default.
• W3161502646 cites W1986287730 @default.
• W3161502646 cites W1990386756 @default.
• W3161502646 cites W2000657683 @default.
• W3161502646 cites W2001281840 @default.
• W3161502646 cites W2006491802 @default.
• W3161502646 cites W2007015054 @default.
• W3161502646 cites W2011177045 @default.
• W3161502646 cites W2026852029 @default.
• W3161502646 cites W2041172302 @default.
• W3161502646 cites W2042172519 @default.
• W3161502646 cites W2043827471 @default.
• W3161502646 cites W2050870661 @default.
• W3161502646 cites W2055750465 @default.
• W3161502646 cites W2063349913 @default.
• W3161502646 cites W2066319384 @default.
• W3161502646 cites W2068813895 @default.
• W3161502646 cites W2069325316 @default.
• W3161502646 cites W2080426384 @default.
• W3161502646 cites W2087655331 @default.
• W3161502646 cites W2088449621 @default.
• W3161502646 cites W2092693142 @default.
• W3161502646 cites W2099559854 @default.
• W3161502646 cites W2104588229 @default.
• W3161502646 cites W2109976702 @default.
• W3161502646 cites W2115213344 @default.
• W3161502646 cites W2116840787 @default.
• W3161502646 cites W2116952160 @default.
• W3161502646 cites W2131427944 @default.
• W3161502646 cites W2137989562 @default.
• W3161502646 cites W2167486498 @default.
• W3161502646 cites W2194639733 @default.
• W3161502646 cites W2525559626 @default.
• W3161502646 cites W2537098252 @default.
• W3161502646 cites W2561823294 @default.
• W3161502646 cites W2588610008 @default.
• W3161502646 cites W2625100576 @default.
• W3161502646 cites W2784284219 @default.
• W3161502646 cites W2798336535 @default.
• W3161502646 cites W2890900272 @default.
• W3161502646 cites W2893947637 @default.
• W3161502646 cites W2901538319 @default.
• W3161502646 cites W2903886915 @default.
• W3161502646 cites W2904495956 @default.
• W3161502646 cites W2947127088 @default.
• W3161502646 cites W2980795582 @default.
• W3161502646 cites W2992990931 @default.
• W3161502646 cites W2996306195 @default.
• W3161502646 cites W3018705847 @default.
• W3161502646 cites W3098002080 @default.
• W3161502646 cites W3098077360 @default.
• W3161502646 cites W3098154307 @default.
• W3161502646 cites W3098594163 @default.
• W3161502646 cites W3098767004 @default.
• W3161502646 cites W3098974664 @default.
• W3161502646 cites W3099093368 @default.
• W3161502646 cites W3099340413 @default.
• W3161502646 cites W3099568156 @default.
• W3161502646 cites W3099724697 @default.
• W3161502646 cites W3100401297 @default.
• W3161502646 cites W3100403874 @default.
• W3161502646 cites W3100441347 @default.
• W3161502646 cites W3100493054 @default.
• W3161502646 cites W3100736846 @default.
• W3161502646 cites W3101282795 @default.
• W3161502646 cites W3101402973 @default.
• W3161502646 cites W3101599961 @default.
• W3161502646 cites W3101779919 @default.
• W3161502646 cites W3101855627 @default.
• W3161502646 cites W3101900982 @default.
• W3161502646 cites W3102054143 @default.
• W3161502646 cites W3102964114 @default.
• W3161502646 cites W3103103352 @default.
• W3161502646 cites W3103681827 @default.
• W3161502646 cites W3104514191 @default.
• W3161502646 cites W3104564178 @default.
• W3161502646 cites W3104610712 @default.
• W3161502646 cites W3105162764 @default.
• W3161502646 cites W3105647453 @default.
• W3161502646 cites W3105941479 @default.
• W3161502646 cites W3109307471 @default.
• W3161502646 cites W3122955073 @default.
• W3161502646 cites W3125052132 @default.
• W3161502646 cites W3147751559 @default.
• W3161502646 cites W4292406582 @default.
• W3161502646 cites W4292951977 @default.
• W3161502646 doi "https://doi.org/10.3847/1538-4357/abe5a6" @default.
• W3161502646 hasPublicationYear "2021" @default.
• W3161502646 type Work @default.
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