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HR4049: signature of nova nucleosynthesis?

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dc.contributor.authorLugaro, Maria A
dc.contributor.authorPols, O.R.
dc.contributor.authorKarakas, Amanda
dc.contributor.authorTout, Christopher A
dc.date.accessioned2015-12-07T22:47:18Z
dc.date.issued2005
dc.date.updated2015-12-07T11:50:28Z
dc.description.abstractThe post-Asymptotic Giant Branch (AGB) star HR4049 is in an eccentric binary system with a relatively short period probably surrounded by a dusty circumbinary disk. Extremely anomalous oxygen isotopic ratios, 16O/17O ≃ 16O/18O ≃ 7, have been measured
dc.identifier.issn0375-9474
dc.identifier.urihttp://hdl.handle.net/1885/26021
dc.publisherElsevier
dc.sourceNuclear Physics A
dc.titleHR4049: signature of nova nucleosynthesis?
dc.typeJournal article
local.bibliographicCitation.lastpage728
local.bibliographicCitation.startpage725
local.contributor.affiliationLugaro, Maria A, University of Cambridge
local.contributor.affiliationPols, O.R., Astronomical Institute Utrecht
local.contributor.affiliationKarakas, Amanda, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationTout, Christopher A, University of Cambridge
local.contributor.authoruidKarakas, Amanda, u4382192
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu3379551xPUB42
local.identifier.citationvolume758
local.identifier.doi10.1016/j.nuclphysa.2005.05.130
local.identifier.scopusID2-s2.0-20944442635
local.type.statusPublished Version

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