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The puzzling white dwarf cooling sequence in NGC 6791: A simple solution

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dc.contributor.authorBedin, L R
dc.contributor.authorSalaris, M
dc.contributor.authorPiotto, G
dc.contributor.authorCassisi, S
dc.contributor.authorMilone, Antonino
dc.contributor.authorAnderson, Jay
dc.contributor.authorKing, I R
dc.date.accessioned2015-12-13T22:54:53Z
dc.date.issued2008
dc.date.updated2015-12-11T11:06:56Z
dc.description.abstractIn this Letter we demonstrate that the puzzling bright peak in the luminosity function of the white dwarf (WD) cooling sequence of NGC 6791 can be naturally accounted for if ∼34% of the observed WDs are WD+WD binary systems.
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/82302
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Open clusters and associations: individual (NGC 6791); White dwarfs
dc.titleThe puzzling white dwarf cooling sequence in NGC 6791: A simple solution
dc.typeJournal article
local.bibliographicCitation.issue1 (PART 2)
local.bibliographicCitation.lastpageL32
local.bibliographicCitation.startpageL29
local.contributor.affiliationBedin, L R, Space Telescope Science Institute
local.contributor.affiliationSalaris, M, Liverpool John Moores University
local.contributor.affiliationPiotto, G, Università di Padova
local.contributor.affiliationCassisi, S, INAF-Observatorio Astronomico di Collurania
local.contributor.affiliationMilone, Antonino, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationAnderson, Jay, Space Telescope Science Institute
local.contributor.affiliationKing, I R, University of Washington
local.contributor.authoruidMilone, Antonino, u5219567
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationf5625xPUB10570
local.identifier.citationvolume679
local.identifier.doi10.1086/589151
local.identifier.scopusID2-s2.0-51949114612
local.type.statusPublished Version

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