Empirical Temperature Measurement in Protoplanetary Disks

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dc.citation.articleNumber113en_US
dc.citation.journalTitleThe Astrophysical Journalen_US
dc.citation.volumeNumber853en_US
dc.contributor.authorWeaver, Eriken_US
dc.contributor.authorIsella, Andreaen_US
dc.contributor.authorBoehler, Yannen_US
dc.date.accessioned2018-07-11T19:50:55Zen_US
dc.date.available2018-07-11T19:50:55Zen_US
dc.date.issued2018en_US
dc.description.abstractThe accurate measurement of temperature in protoplanetary disks is critical to understanding many key features of disk evolution and planet formation, from disk chemistry and dynamics, to planetesimal formation. This paper explores the techniques available to determine temperatures from observations of single, optically thick molecular emission lines. Specific attention is given to issues such as the inclusion of optically thin emission, problems resulting from continuum subtraction, and complications of real observations. Effort is also made to detail the exact nature and morphology of the region emitting a given line. To properly study and quantify these effects, this paper considers a range of disk models, from simple pedagogical models to very detailed models including full radiative transfer. Finally, we show how the use of the wrong methods can lead to potentially severe misinterpretations of data, leading to incorrect measurements of disk temperature profiles. We show that the best way to estimate the temperature of emitting gas is to analyze the line peak emission map without subtracting continuum emission. Continuum subtraction, which is commonly applied to observations of line emission, systematically leads to underestimation of the gas temperature. We further show that once observational effects such as beam dilution and noise are accounted for, the line brightness temperature derived from the peak emission is reliably within 10%–15% of the physical temperature of the emitting region, assuming optically thick emission. The methodology described in this paper will be applied in future works to constrain the temperature, and related physical quantities, in protoplanetary disks observed with ALMA.en_US
dc.identifier.citationWeaver, Erik, Isella, Andrea and Boehler, Yann. "Empirical Temperature Measurement in Protoplanetary Disks." <i>The Astrophysical Journal,</i> 853, (2018) IOP Publishing: https://doi.org/10.3847/1538-4357/aaa481.en_US
dc.identifier.doihttps://doi.org/10.3847/1538-4357/aaa481en_US
dc.identifier.urihttps://hdl.handle.net/1911/102402en_US
dc.language.isoengen_US
dc.publisherIOP Publishingen_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.titleEmpirical Temperature Measurement in Protoplanetary Disksen_US
dc.typeJournal articleen_US
dc.type.dcmiTexten_US
dc.type.publicationpublisher versionen_US
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