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Tracing the Development of Dust around Evolved Stars: The Case of 47 Tuc.

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dc.contributor.authorLebeltzer, Th.
dc.contributor.authorPosch, Th.
dc.contributor.authorHinkle, Kenneth H
dc.contributor.authorWood, Peter R
dc.contributor.authorBouwman, J.
dc.date.accessioned2015-12-07T22:21:12Z
dc.date.issued2006
dc.date.updated2015-12-07T08:54:53Z
dc.description.abstractWe observed mid-infrared (7.5-22 μm) spectra of asymptotic giant branch (AGB) stars in the globular cluster 47 Tuc with the Spitzer Space Telescope, and we find significant dust features of various types. A comparison of the characteristics of the dust s
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/19931
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Stars: AGB and post-AGB; Stars: evolution; Stars: mass loss
dc.titleTracing the Development of Dust around Evolved Stars: The Case of 47 Tuc.
dc.typeJournal article
local.bibliographicCitation.lastpage48
local.bibliographicCitation.startpageL145
local.contributor.affiliationLebeltzer, Th., Institut fur Astronomie
local.contributor.affiliationPosch, Th., Institut fur Astronomie
local.contributor.affiliationHinkle, Kenneth H, National Optical Astronomy Observatory
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBouwman, J., Max Planck Institute for Astronomy
local.contributor.authoruidWood, Peter R, u7900259
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4370312xPUB10
local.identifier.citationvolume653
local.identifier.doi10.1086/510525
local.identifier.scopusID2-s2.0-33846363505
local.type.statusPublished Version

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