Rotating and magnetic stellar models of intermediate-mass stars up to the AGB

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dc.creatorLuiz Themystokliz Sanctos Mendes
dc.creatorNatália R. Landin
dc.creatorPaolo Ventura
dc.date.accessioned2025-04-15T15:09:10Z
dc.date.accessioned2025-09-08T23:24:07Z
dc.date.available2025-04-15T15:09:10Z
dc.date.issued2018
dc.identifier.doihttps://doi.org/10.1017/S1743921318006051
dc.identifier.issn1743-9213
dc.identifier.urihttps://hdl.handle.net/1843/81608
dc.languageeng
dc.publisherUniversidade Federal de Minas Gerais
dc.relation.ispartofProceedings of The Inernational Astronomical Union
dc.rightsAcesso Restrito
dc.subjectEstrelas - Evolução
dc.subject.otherstars: evolution
dc.subject.otherstars: rotation
dc.subject.otherstars: interiors
dc.titleRotating and magnetic stellar models of intermediate-mass stars up to the AGB
dc.typeArtigo de evento
local.citation.epage469
local.citation.spage468
local.description.resumoAiming at investigating the roles of rotation and magnetic fields on AGB stars, the rotating version of the ATON stellar evolution code is being extended in order to account for intermediate--mass stars and their later evolutionary stages. Here we report some preliminary results on the effects of rotation and of a large-scale magnetic field on the structure and evolution of 3 and 5 M⊙ stellar models from the pre-main sequence up to the AGB.
local.publisher.countryBrasil
local.publisher.departmentENG - DEPARTAMENTO DE ENGENHARIA ELETRÔNICA
local.publisher.departmentICX - DEPARTAMENTO DE MATEMÁTICA
local.publisher.initialsUFMG
local.url.externahttps://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/rotating-and-magnetic-stellar-models-of-intermediatemass-stars-up-to-the-agb/01AE3F2C51B615BD268C4E1E6F320FE7

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