Modules for experiments in Stellar Astrophysics (MESA): Planets, oscillations, rotation, and massive stars

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dc.contributor.authorPaxton, Bill
dc.contributor.authorCantiello, Matteo
dc.contributor.authorArras, Phil
dc.contributor.authorBildsten, Lars
dc.contributor.authorBrown, E.F.
dc.contributor.authorDotter, Aaron
dc.contributor.authorMankovich, Christopher
dc.contributor.authorMontgomery, M H
dc.contributor.authorStello, Dennis
dc.contributor.authorTimmes, F X
dc.contributor.authorTownsend, Richard
dc.date.accessioned2015-12-13T22:30:23Z
dc.date.issued2013
dc.date.updated2016-02-24T09:23:45Z
dc.description.abstractWe substantially update the capabilities of the open source software package Modules for Experiments in Stellar Astrophysics (MESA), and its one-dimensional stellar evolution module, MESA star. Improvements in MESA star's ability to model the evolution of
dc.identifier.issn0067-0049
dc.identifier.urihttp://hdl.handle.net/1885/74814
dc.publisherInstitute of Physics Publishing
dc.sourceAstrophysical Journal Supplement Series
dc.subjectKeywords: asteroseismology; methods: numerical; planets and satellites: physical evolution; stars: evolution; stars: massive; stars: rotation
dc.titleModules for experiments in Stellar Astrophysics (MESA): Planets, oscillations, rotation, and massive stars
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.startpage4
local.contributor.affiliationPaxton, Bill, University of California
local.contributor.affiliationCantiello, Matteo, University of California
local.contributor.affiliationArras, Phil, University of Virginia
local.contributor.affiliationBildsten, Lars, University of California
local.contributor.affiliationBrown, E.F., Michigan State University
local.contributor.affiliationDotter, Aaron, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMankovich, Christopher, University of California
local.contributor.affiliationMontgomery, M H, University of Texas
local.contributor.affiliationStello, Dennis, University of Sydney
local.contributor.affiliationTimmes, F X, Arizona State University
local.contributor.affiliationTownsend, Richard, University of Wisconsin-Madison
local.contributor.authoremailu5239381@anu.edu.au
local.contributor.authoruidDotter, Aaron, u5239381
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB4317
local.identifier.citationvolume208
local.identifier.doi10.1088/0067-0049/208/1/4
local.identifier.scopusID2-s2.0-84884221944
local.identifier.thomsonID000324172700004
local.identifier.uidSubmittedByf5625
local.type.statusPublished Version

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