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dc.contributor.authorRyan, Sean G.
dc.date.accessioned2007-08-11T19:40:51Z
dc.date.available2007-08-11T19:40:51Z
dc.date.issued2002
dc.identifier.citationRyan , S G 2002 , ' Big Bang Nucleosynthesis, Population III, and Stellar Genetics in the Galactic Halo ' , Publications of the Astronomical Society of Australia , vol. 19 , no. 2 , pp. 238-245 . https://doi.org/10.1071/AS01067
dc.identifier.issn1323-3580
dc.identifier.otherPURE: 170850
dc.identifier.otherPURE UUID: aa9210a1-9145-448e-bacd-4131a0941e35
dc.identifier.otherdspace: 2299/326
dc.identifier.otherScopus: 29144464499
dc.identifier.otherORCID: /0000-0001-9069-5122/work/30501366
dc.identifier.urihttp://hdl.handle.net/2299/326
dc.descriptionOriginal article can be found at: http://www.publish.csiro.au --Copyright CSIRO --DOI : 10.1071/AS01067
dc.description.abstractThe diverse isotopic and elemental signatures produced in different nucle- osynthetic sites are passed on to successive generations of stars. By tracing these chemical signatures back through the stellar populations of the Galaxy, it is pos- sible to unravel its nucleosynthetic history and even to study stars which are now extinct. This review considers recent applications of ”stellar genetics” to examine the earliest episodes of nucleosynthesis in the Universe, in Population III stars and the Big Bang.en
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of Australia
dc.titleBig Bang Nucleosynthesis, Population III, and Stellar Genetics in the Galactic Haloen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1071/AS01067
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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