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The derivation of pulsation velocities from Doppler line profiles in M-type Mira variables

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dc.contributor.authorScholz, M
dc.contributor.authorWood, Peter R
dc.date.accessioned2015-12-08T22:43:03Z
dc.date.available2015-12-08T22:43:03Z
dc.date.issued2000
dc.date.updated2015-12-08T10:37:55Z
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/37113
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.titleThe derivation of pulsation velocities from Doppler line profiles in M-type Mira variables
dc.typeJournal article
local.bibliographicCitation.lastpage1071
local.bibliographicCitation.startpage1065
local.contributor.affiliationScholz, M, University of Sydney
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidWood, Peter R, u7900259
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub145
local.identifier.citationvolume362
local.type.statusPublished Version

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