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dc.contributor.authorWoitke, Peter
dc.date.accessioned2015-10-02T16:10:02Z
dc.date.available2015-10-02T16:10:02Z
dc.date.issued2015-09-23
dc.identifier.citationWoitke , P 2015 , ' Modelling and interpretation of SEDs ' , EPJ Web of Conferences , vol. 102 , 00007 . https://doi.org/10.1051/epjconf/201510200007en
dc.identifier.issn2100-014X
dc.identifier.otherPURE: 220993214
dc.identifier.otherPURE UUID: 1d3ebea5-c032-40b1-9c60-018fcff478d6
dc.identifier.otherBibtex: urn:d965ac09cfd8cf0b1f54ba26ea999bf5
dc.identifier.otherScopus: 84960112482
dc.identifier.otherWOS: 000372793100006
dc.identifier.urihttps://hdl.handle.net/10023/7589
dc.descriptionThe research leading to these results has received funding from the European Union Seventh Framework Programme FP7-2011 under grant agreement no 284405. 6th Lecture from Summer School “Protoplanetary Disks: Theory and Modelling Meet Observations”en
dc.description.abstractCircumstellar disks are mostly detected by larger continuum fluxes in the infrared to mm spectral regions as compared to naked stars (a flux excess). The analysis of the Spectral Energy Distribution (SED) of that flux excess was crucial for the development of the first theories about protoplanetary disks, and even nowadays, it is still one of the major tools to physically characterise the disks in terms of their mass, inner holes and gaps, vertical extension & shape, dust properties, and evolutionary state. In this chapter, we will review some of the early simple theories, show some examples, discuss the influence of typical disk shape and dust size parameters in modern SED analysis, and discuss how degenerate the results can be.
dc.format.extent24
dc.language.isoeng
dc.relation.ispartofEPJ Web of Conferencesen
dc.rights© Owned by author, published by EDP Sciences, 2015. This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.en
dc.subjectQC Physicsen
dc.subjectT-NDASen
dc.subject.lccQCen
dc.titleModelling and interpretation of SEDsen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1051/epjconf/201510200007
dc.description.statusPeer revieweden


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