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Spread of the dust temperature distribution in circumstellar disks

dc.contributor.authorHEESE, S.
hal.structure.identifierLaboratoire de tectonique [LT]
dc.contributor.authorWOLF, S.
hal.structure.identifierAMOR 2017
dc.contributor.authorDUTREY, Anne
hal.structure.identifierAMOR 2017
dc.contributor.authorGUILLOTEAU, S.
dc.date.issued2017-05
dc.identifier.issn0004-6361
dc.description.abstractEnAccurate temperature calculations for circumstellar disks are particularly important for their chemical evolution. Their temperature distribution is determined by the optical properties of the dust grains, which, among other parameters, depend on their radius. However, in most disk studies, only average optical properties and thus an average temperature is assumed to account for an ensemble of grains with different radii. We investigate the impact of subdividing the grain radius distribution into multiple sub-intervals on the resulting dust temperature distribution and spectral energy distribution (SED). These quantities were computed for two different scenarios: (1) Radius distribution represented by 16 logarithmically distributed radius intervals, and (2) radius distribution represented by a single grain species with averaged optical properties (reference). Within the considered parameter range, i.e., of grain radii between 5 nm and 1 mm and an optically thin and thick disk with a parameterized density distribution, we obtain the following results: In optically thin disk regions, the temperature spread can be as large as ~63% and the relative grain surface below a certain temperature is lower than in the reference disk. With increasing optical depth, the difference in the midplane temperature and the relative grain surface below a certain temperature decreases. Furthermore, below ~20K, this fraction is higher for the reference disk than for the case of multiple grain radii, while it shows the opposite behavior for temperatures above this threshold. The thermal emission in the case of multiple grain radii at short wavelengths is stronger than for the reference disk. The freeze-out radius is a function of grain radius, spanning a radial range between the coldest and warmest grain species of ~30AU.
dc.language.isoen
dc.publisherEDP Sciences
dc.rights.urihttp://creativecommons.org/licenses/by/
dc.subject.enAstrophysics - Earth and Planetary Astrophysics
dc.subject.enAstrophysics - Solar and Stellar Astrophysics
dc.title.enSpread of the dust temperature distribution in circumstellar disks
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/201730501
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageA5
bordeaux.volume604
bordeaux.peerReviewedoui
hal.identifierhal-01519704
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01519704v1
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