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Copious amounts of hot and cold dust orbiting the main sequence A-type stars HD 131488 and HD 121191

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dc.contributor.authorMelis, C
dc.contributor.authorZuckerman, B
dc.contributor.authorRhee, Joseph H
dc.contributor.authorSong, Inseok
dc.contributor.authorMurphy, Simon
dc.contributor.authorBessell, Michael
dc.date.accessioned2015-12-13T22:32:20Z
dc.date.issued2013
dc.date.updated2015-12-11T09:06:18Z
dc.description.abstractWe report two new dramatically dusty main sequence stars: HD 131488 (A1 V) and HD 121191 (A8 V). HD 131488 is found to have substantial amounts of dust in its terrestrial planet zone (L IR/L bol ≈ 4 × 10-3), cooler dust farther out in its planetary sys
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/75517
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.titleCopious amounts of hot and cold dust orbiting the main sequence A-type stars HD 131488 and HD 121191
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1
local.bibliographicCitation.startpage8
local.contributor.affiliationMelis, C, University of California
local.contributor.affiliationZuckerman, B, University of California
local.contributor.affiliationRhee, Joseph H, California State Polytechnic University
local.contributor.affiliationSong, Inseok, University of Georgia
local.contributor.affiliationMurphy, Simon, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBessell, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidMurphy, Simon, u4203307
local.contributor.authoruidBessell, Michael, u6900904
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB4655
local.identifier.citationvolume778
local.identifier.doi10.1088/0004-637X/778/1/12
local.identifier.scopusID2-s2.0-84887572859
local.identifier.thomsonID000327131700012
local.type.statusPublished Version

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