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Ionization cone in the X-ray binary LMC X-1

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dc.contributor.authorCooke, R
dc.contributor.authorBland-Hawthorn, Joss
dc.contributor.authorSharp, Robert
dc.contributor.authorKuncic, Zdenka
dc.date.accessioned2015-12-13T22:55:28Z
dc.date.issued2008
dc.date.updated2015-12-11T11:10:45Z
dc.description.abstractIn an earlier paper, we presented the first evidence for a bow-shock nebula surrounding the X-ray binary LMC X-1 on a scale of ∼15 pc, which we argued was powered by a jet associated with an accretion disk. We now present the first evidence for an ioniz
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/82545
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.titleIonization cone in the X-ray binary LMC X-1
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpageL32
local.bibliographicCitation.startpageL29
local.contributor.affiliationCooke, R, University of Sydney
local.contributor.affiliationBland-Hawthorn, Joss, University of Sydney
local.contributor.affiliationSharp, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationKuncic, Zdenka , University of Sydney
local.contributor.authoruidSharp, Robert, u4954956
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationf5625xPUB10801
local.identifier.citationvolume687
local.identifier.scopusID2-s2.0-70350753078
local.identifier.thomsonID000262731800008
local.type.statusPublished Version

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