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The K-Band Intensity Profile of R Leonis Probed by VLTI/VINCI

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dc.contributor.authorFedele, D
dc.contributor.authorWittkowski, M
dc.contributor.authorParesce, F
dc.contributor.authorScholz, Michael
dc.contributor.authorWood, Peter R
dc.contributor.authorCiroi, S
dc.date.accessioned2015-12-08T22:24:49Z
dc.date.available2015-12-08T22:24:49Z
dc.date.issued2008
dc.date.updated2015-12-08T08:59:40Z
dc.description.abstractWe present near-infrared K-band interferometric measurements of the Mira star R Leonis obtained in April 2001 and January 2002 with VLTI/VINCI. The April 2001 measurements indicate a center-to-limb intensity variation (CLV) that is clearly different from
dc.identifier.isbn9783540742531
dc.identifier.urihttp://hdl.handle.net/1885/33160
dc.publisherSpringer
dc.relation.ispartofThe Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation
dc.relation.isversionof1st Edition
dc.titleThe K-Band Intensity Profile of R Leonis Probed by VLTI/VINCI
dc.typeBook chapter
local.bibliographicCitation.lastpage98
local.bibliographicCitation.placeofpublicationHeidelberg
local.bibliographicCitation.startpage95
local.contributor.affiliationFedele, D, European Southern Observatory
local.contributor.affiliationWittkowski, M, European Southern Observatory
local.contributor.affiliationParesce, F, European Southern Observatory
local.contributor.affiliationScholz, Michael, University of Heidelberg
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationCiroi, S, Universita di Padova
local.contributor.authoruidWood, Peter R, u7900259
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4362859xPUB99
local.identifier.doi10.1007/978-3-540-74256-2_10
local.identifier.scopusID2-s2.0-35448983562
local.type.statusPublished Version

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