Abundance Analysis of New CEMP RR Lyrae Stars

Kennedy, C. R.

A change is coming. Click to see a sneak peek of the new Open Research Repository.

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

Download

There are no files associated with this item.

Show simple item record