HR4049: signature of nova nucleosynthesis?
dc.contributor.author | Lugaro, Maria A | |
dc.contributor.author | Pols, O.R. | |
dc.contributor.author | Karakas, Amanda | |
dc.contributor.author | Tout, Christopher A | |
dc.date.accessioned | 2015-12-07T22:47:18Z | |
dc.date.issued | 2005 | |
dc.date.updated | 2015-12-07T11:50:28Z | |
dc.description.abstract | The 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.issn | 0375-9474 | |
dc.identifier.uri | http://hdl.handle.net/1885/26021 | |
dc.publisher | Elsevier | |
dc.source | Nuclear Physics A | |
dc.title | HR4049: signature of nova nucleosynthesis? | |
dc.type | Journal article | |
local.bibliographicCitation.lastpage | 728 | |
local.bibliographicCitation.startpage | 725 | |
local.contributor.affiliation | Lugaro, Maria A, University of Cambridge | |
local.contributor.affiliation | Pols, O.R., Astronomical Institute Utrecht | |
local.contributor.affiliation | Karakas, Amanda, College of Physical and Mathematical Sciences, ANU | |
local.contributor.affiliation | Tout, Christopher A, University of Cambridge | |
local.contributor.authoremail | u4382192@anu.edu.au | |
local.contributor.authoruid | Karakas, Amanda, u4382192 | |
local.description.embargo | 2037-12-31 | |
local.description.notes | Imported from ARIES | |
local.identifier.absfor | 020110 - Stellar Astronomy and Planetary Systems | |
local.identifier.ariespublication | u3379551xPUB42 | |
local.identifier.citationvolume | 758 | |
local.identifier.doi | 10.1016/j.nuclphysa.2005.05.130 | |
local.identifier.scopusID | 2-s2.0-20944442635 | |
local.identifier.uidSubmittedBy | u3379551 | |
local.type.status | Published Version |
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