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Spatially resolving the accretion shocks on the rapidly-rotating M0 T-Tauri star MN Lupi

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dc.contributor.authorStrassmeier, K G
dc.contributor.authorRice, J B
dc.contributor.authorRitter, A
dc.contributor.authorKuker, M
dc.contributor.authorHussain, G
dc.contributor.authorHubrig, S
dc.contributor.authorShobbrook, R
dc.date.accessioned2015-12-13T22:54:41Z
dc.date.issued2005
dc.date.updated2015-12-11T11:05:35Z
dc.description.abstractWe obtained high-resolution, high-quality VLT/UVES spectra to reconstruct the two-dimensional surface structure of the rapidly-rotating classical T-Tauri star MN Lupi on two separate nights. Both surface maps show a structured warm (5000 K) band centered
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/82204
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Imaging techniques; Magnetic field effects; Magnetosphere; Maps; Mathematical models; Spectroscopic analysis; Stars: activity; Stars: imaging; Stars: individual: MN Lup; Stars: individual: T Tauri; Stars: pre-main sequence; Starspots; Astrophysics Stars: activity; Stars: imaging; Stars: individual: MN Lup; Stars: individual: T Tauri; Stars: pre-main sequence; Starspots
dc.titleSpatially resolving the accretion shocks on the rapidly-rotating M0 T-Tauri star MN Lupi
dc.typeJournal article
local.bibliographicCitation.lastpage1118
local.bibliographicCitation.startpage1105
local.contributor.affiliationStrassmeier, K G, Astrophysical Institute Potsdam
local.contributor.affiliationRice, J B, University of Brandon
local.contributor.affiliationRitter, A, Astrophysical Institute Potsdam
local.contributor.affiliationKuker, M, Astrophysical Institute Potsdam
local.contributor.affiliationHussain, G, Harvard-Smithsonian Center for Astrophysics
local.contributor.affiliationHubrig, S, European Southern Observatory
local.contributor.affiliationShobbrook, R, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidShobbrook, R, u4010450
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub10478
local.identifier.citationvolume440
local.identifier.doi10.1051/0004-6361:20052901
local.identifier.scopusID2-s2.0-25444455650
local.type.statusPublished Version

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