Abundance Analysis of New CEMP RR Lyrae Stars
Description
Tonight, in the halo of the Galaxy, we observe variable carbon-enhanced metal-poor stars. These stars preserve chemical signatures of past stellar nucleosynthesis. We will use the WiFeS instrument in order to estimate accurate abundances of several elements. By doing so, we will determine how the first generations of stars produced the elements that surround us.
dc.contributor.author | Kennedy, C. R. | |
---|---|---|
dc.coverage.temporal | From 2013-03-20 12:00:00 To 2013-03-22 12:00:00 | |
dc.date.accessioned | 2018-09-14T03:11:11Z | |
dc.date.available | 2018-09-14T03:11:11Z | |
dc.date.created | 2013 | |
dc.identifier.uri | http://hdl.handle.net/1885/147473 | |
dc.description.abstract | Tonight, in the halo of the Galaxy, we observe variable carbon-enhanced metal-poor stars. These stars preserve chemical signatures of past stellar nucleosynthesis. We will use the WiFeS instrument in order to estimate accurate abundances of several elements. By doing so, we will determine how the first generations of stars produced the elements that surround us. | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_AU | |
dc.publisher | Canberra, ACT: The Australian National University Data Commons | |
dc.rights | Author/s retain copyright | |
dc.source.uri | https://datacommons.anu.edu.au/DataCommons/item/anudc:5032 | |
dc.source.uri | https://researchdata.ands.org.au/abundance-analysis-new-lyrae-stars | |
dc.subject | Astronomical and Space Sciences | |
dc.subject | Physical Sciences | |
dc.title | Abundance Analysis of New CEMP RR Lyrae Stars | |
dc.type | Dataset | |
local.type.status | Metadata only | |
dcterms.accessRights | Open Access via publisher website | |
dc.rights.license | All data obtained on ANU telescopes is publicly available after 12 months. Please contact the PI to negotiate access before that time. | |
Collections | ANU Research Publications |
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