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Dynamical mass of the substellar benchmark binary HD 130948BC

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dc.contributor.authorDupuy, Trent Jen_AU
dc.contributor.authorLiu, Michael Cen_AU
dc.contributor.authorIreland, Michaelen_AU
dc.date.accessioned2015-12-10T23:24:00Z
dc.date.issued2009
dc.date.updated2016-02-24T09:59:35Z
dc.description.abstractWe present Keck adaptive optics imaging of the L4+L4 binary HD 130948BC along with archival Hubble Space Telescope and Gemini North observations, which together span ≈ 70% of the binary's orbital period. From the relative orbit, we determine a total dyn
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/67050
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Binaries: close; Binaries: general; Infrared: stars; Stars: low-mass brown dwarfs; Techniques: high angular resolution
dc.titleDynamical mass of the substellar benchmark binary HD 130948BC
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage752
local.bibliographicCitation.startpage729
local.contributor.affiliationDupuy, Trent J, University of Hawaii
local.contributor.affiliationLiu, Michael C, University of Hawaii
local.contributor.affiliationIreland, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidIreland, Michael, u5544212
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationU3488905xPUB1388
local.identifier.citationvolume692
local.identifier.doi10.1088/0004-637X/692/1/729
local.identifier.scopusID2-s2.0-77954567780
local.type.statusPublished Version

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