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Very Large Telescope three micron spectra of dust-enshrouded red giants in the Large Magellanic Cloud

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dc.contributor.authorvan Loon, Jacco Th
dc.contributor.authorMarshall, J R
dc.contributor.authorCohen, Marvin L.
dc.contributor.authorMatsuura, Mikako
dc.contributor.authorWood, Peter R
dc.contributor.authorYamamura, I
dc.contributor.authorZijlstra, Albert A
dc.date.accessioned2015-12-07T22:21:45Z
dc.date.issued2006
dc.date.updated2015-12-07T09:01:08Z
dc.description.abstractWe present ESO/VLT spectra in the 2.9-4.1 μm range for a large sample of infrared stars in the Large Magellanic Cloud (LMC), selected on the basis of MSX and 2MASS colours to be extremely dust-enshrouded AGB star candidates. Out of 30 targets, 28 are pos
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/20174
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Absorption; Astrophysics; Carbon; Galaxies; Circumstellar matter; Infrared: stars; Magellanic Clouds; Stars: AGB and post-AGB; Stars: carbon; Stars: mass-loss; Telescopes Circumstellar matter; Infrared: stars; Magellanic Clouds; Stars: AGB and post-AGB; Stars: carbon; Stars: mass-loss
dc.titleVery Large Telescope three micron spectra of dust-enshrouded red giants in the Large Magellanic Cloud
dc.typeJournal article
local.bibliographicCitation.lastpage989
local.bibliographicCitation.startpage971
local.contributor.affiliationvan Loon, Jacco Th, Keele University
local.contributor.affiliationMarshall, J R, Keele University
local.contributor.affiliationCohen, Marvin L., University of California
local.contributor.affiliationMatsuura, Mikako, University of Manchester
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationYamamura, I, Japan Aerospace Exploration Agency
local.contributor.affiliationZijlstra, Albert A, University of Manchester
local.contributor.authoruidWood, Peter R, u7900259
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4370312xPUB11
local.identifier.citationvolume447
local.identifier.doi10.1051/0004-6361:20054222
local.identifier.scopusID2-s2.0-33644510176
local.type.statusPublished Version

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