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Detailed abundances of planet-hosting wide binaries. I. Did planet formation imprint chemical signatures in the atmospheres of HD 20782/81?

dc.contributor.authorMack III, Claude
dc.contributor.authorSchuler, Simon
dc.contributor.authorStassun, Keivan
dc.contributor.authorNorris, John
dc.date.accessioned2015-12-13T22:16:07Z
dc.date.issued2014
dc.date.updated2015-12-11T07:22:53Z
dc.description.abstractUsing high-resolution, high signal-to-noise echelle spectra obtained with Magellan/MIKE, we present a detailed chemical abundance analysis of both stars in the planet-hosting wide binary system HD 20782 + HD 20781. Both stars are G dwarfs, and presumably
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/70715
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.titleDetailed abundances of planet-hosting wide binaries. I. Did planet formation imprint chemical signatures in the atmospheres of HD 20782/81?
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage8
local.bibliographicCitation.startpage1
local.contributor.affiliationMack III, Claude, Vanderbilt University
local.contributor.affiliationSchuler, Simon, University of Tampa
local.contributor.affiliationStassun, Keivan, Vanderbilt University
local.contributor.affiliationNorris, John, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidNorris, John, u7401084
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationU3488905xPUB2390
local.identifier.citationvolume787
local.identifier.doi10.1088/0004-637X/787/2/98
local.identifier.scopusID2-s2.0-84901020688
local.identifier.thomsonID000336246700003
local.type.statusPublished Version

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