Resolving Stellar Atmospheres 1. Hα line and comparisons to microlensing observations

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dc.contributor.authorThurl, Christine
dc.contributor.authorSackett, Penny
dc.contributor.authorHauschildt, Peter H
dc.date.accessioned2015-12-07T22:17:00Z
dc.date.issued2006
dc.date.updated2015-12-07T08:00:57Z
dc.description.abstractContext. We present work on Hα spectral line characteristics in PHOENIX stellar model atmospheres and their comparison to microlensing observations. Aims. We examine in detail the Ha equivalent width (EW) and the line shape characteristics for effective
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/18334
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Absorption; Parameter estimation; Thermodynamics; Chromospheric emission; Gravitational lensing; Stars: atmospheres; Thermodynamic equilibrium (LTE); Astronomy Gravitational lensing; Stars: atmospheres
dc.titleResolving Stellar Atmospheres 1. Hα line and comparisons to microlensing observations
dc.typeJournal article
local.bibliographicCitation.lastpage324
local.bibliographicCitation.startpage315
local.contributor.affiliationThurl, Christine, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSackett, Penny, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationHauschildt, Peter H, Hamburger Sternwarte
local.contributor.authoruidThurl, Christine, u2573208
local.contributor.authoruidSackett, Penny, u4049146
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4114753xPUB4
local.identifier.citationvolume455
local.identifier.doi10.1051/0004-6361:20054766
local.identifier.scopusID2-s2.0-33747460315
local.type.statusPublished Version

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