Determining the origin of inner planetary system debris orbiting the dustiest main sequence stars

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dc.contributor.authorMelis, Carlen
dc.contributor.authorZuckerman, B.en
dc.contributor.authorRhee, Joseph H.en
dc.contributor.authorSong, Inseoken
dc.contributor.authorMurphy, S. J.en
dc.contributor.authorBessell, M. S.en
dc.date.accessioned2026-01-01T08:41:22Z
dc.date.available2026-01-01T08:41:22Z
dc.date.issued2012en
dc.description.abstractWe develop a means to distinguish between warm dusty circumstellar debris disks produced by steady state collisional evolution of a planetesimal belt or through transient events.en
dc.description.statusPeer-revieweden
dc.format.extent5en
dc.identifier.isbn9781107033825en
dc.identifier.issn1743-9213en
dc.identifier.scopus84899871677en
dc.identifier.urihttps://hdl.handle.net/1885/733799065
dc.language.isoenen
dc.publisherCambridge University Pressen
dc.relation.ispartofFormation, Detection, and Characterization of Extrasolar Habitable Planetsen
dc.relation.ispartofseriesProceedings of the International Astronomical Unionen
dc.relation.isversionofS293en
dc.subjectcircumstellar matteren
dc.subjectplanetary systems: formationen
dc.subjectplanets and satellites: formationen
dc.titleDetermining the origin of inner planetary system debris orbiting the dustiest main sequence starsen
dc.typeConference paperen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage277en
local.bibliographicCitation.startpage273en
local.contributor.affiliationMelis, Carl; University of California at San Diegoen
local.contributor.affiliationZuckerman, B.; University of California at Los Angelesen
local.contributor.affiliationRhee, Joseph H.; California State Polytechnic University Pomonaen
local.contributor.affiliationSong, Inseok; University of Georgiaen
local.contributor.affiliationMurphy, S. J.; RSAA - Stromlo, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationBessell, M. S.; RSAA - Stromlo, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.identifier.ariespublicationu4830877xPUB71en
local.identifier.doi10.1017/S1743921313012970en
local.identifier.essn1743-9221en
local.identifier.pure5e110fc9-0fd8-4c4e-8476-ea43d31a9ec4en
local.identifier.urlhttps://www.scopus.com/pages/publications/84899871677en
local.type.statusPublisheden

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