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dc.contributor.authorHubeny, Ivan
dc.date.accessioned2017-06-27T16:21:12Z
dc.date.available2017-06-27T16:21:12Z
dc.date.issued2017-07
dc.identifier.citationModel atmospheres of sub-stellar mass objects 2017, 469 (1):841 Monthly Notices of the Royal Astronomical Societyen
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.doi10.1093/mnras/stx758
dc.identifier.urihttp://hdl.handle.net/10150/624422
dc.description.abstractWe present an outline of basic assumptions and governing structural equations describing atmospheres of sub-stellar mass objects, in particular the extrasolar giant planets and brown dwarfs. Although most of the presentation of the physical and numerical background is generic, details of the implementation pertain mostly to the code COOLTLUSTY. We also present a review of numerical approaches and computer codes devised to solve the structural equations, and make a critical evaluation of their efficiency and accuracy.
dc.description.sponsorshipSackler Distinguished Visitor program of the Institute of Astronomy at the University of Cambridgeen
dc.language.isoenen
dc.publisherOXFORD UNIV PRESSen
dc.relation.urlhttps://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stx758en
dc.rights© 2017 The Author Published by Oxford University Press on behalf of the Royal Astronomical Societyen
dc.subjectRadiative Transferen
dc.subjectmethods: numericalen
dc.subjectplanets and satellites: atmospheresen
dc.subjectbrown dwarfsen
dc.titleModel atmospheres of sub-stellar mass objectsen
dc.typeArticleen
dc.contributor.departmentUniv Arizona, Steward Observen
dc.identifier.journalMonthly Notices of the Royal Astronomical Societyen
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en
dc.eprint.versionFinal published versionen
refterms.dateFOA2018-09-11T20:32:59Z
html.description.abstractWe present an outline of basic assumptions and governing structural equations describing atmospheres of sub-stellar mass objects, in particular the extrasolar giant planets and brown dwarfs. Although most of the presentation of the physical and numerical background is generic, details of the implementation pertain mostly to the code COOLTLUSTY. We also present a review of numerical approaches and computer codes devised to solve the structural equations, and make a critical evaluation of their efficiency and accuracy.


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