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On the Shock-induced Variability of Emission Lines in M-type Mira Variables II. FeII and [FeII] emission lines as a diagnostic tool

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dc.contributor.authorRichter, He
dc.contributor.authorWood, Peter R
dc.contributor.authorWoitke, P
dc.contributor.authorBolick, U.
dc.contributor.authorSedlmayr, E
dc.date.accessioned2015-12-13T23:09:40Z
dc.date.available2015-12-13T23:09:40Z
dc.date.issued2003
dc.date.updated2015-12-12T08:20:11Z
dc.description.abstractOur observations of cool, shock penetrated, expanding atmospheres of M-type Mira variables (Richter & Wood 2001) have suggested that the emission lines of Fe II and [Fe II] can serve as an excellent diagnostic tool to study the hydro- and thermodynamical
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/87101
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Calculations; Galaxies; Hydrodynamics; Ionization; Light emission; Mathematical models; Shock waves; Thermodynamics; Nonlocal thermodynamic equilibrium; Photosphere; Radiative transfer; Astrophysics Line: Formation; Radiative transfer; Shock waves; Stars: Late-type; Stars: Variables: General
dc.titleOn the Shock-induced Variability of Emission Lines in M-type Mira Variables II. FeII and [FeII] emission lines as a diagnostic tool
dc.typeJournal article
local.bibliographicCitation.lastpage328
local.bibliographicCitation.startpage319
local.contributor.affiliationRichter, He, Berlin Institute of Technology
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWoitke, P, Berlin Institute of Technology
local.contributor.affiliationBolick, U., Berlin Institute of Technology
local.contributor.affiliationSedlmayr, E, Berlin Institute of Technology
local.contributor.authoruidWood, Peter R, u7900259
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16240
local.identifier.citationvolume400
local.identifier.scopusID2-s2.0-0037337735
local.type.statusPublished Version

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