CHEMICAL SIGNATURES OF THE FIRST SUPERNOVAE IN THE SCULPTOR DWARF SPHEROIDAL GALAXY

We present a homogeneous chemical abundance analysis of five of the most metal-poor stars in the Sculptor dwarf spheroidal galaxy. We analyze new and archival high resolution spectroscopy from Magellan/MIKE and VLT/UVES and determine stellar parameters and abundances in a consistent way for each sta...

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Bibliographic Details
Main Authors: Simon, Joshua D., Jacobson, Heather, Thompson, Ian B., Adams, Joshua J., Shectman, Stephen A., Frebel, Anna L.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: IOP Publishing 2015
Online Access:http://hdl.handle.net/1721.1/97092
https://orcid.org/0000-0001-7727-1640
https://orcid.org/0000-0002-2139-7145