HUBBLE SPACE TELESCOPE NEAR-ULTRAVIOLET SPECTROSCOPY OF BRIGHT CEMP-s STARS

We present an elemental-abundance analysis, in the near-ultraviolet (NUV) spectral range, for the bright carbon-enhanced metal-poor (CEMP) stars HD 196944 (V = 8.40, [Fe/H] = −2.41) and HD 201626 (V = 8.16, [Fe/H] = −1.51), based on data acquired with the Space Telescope Imaging Spectrograph (STIS)...

Full description

Bibliographic Details
Main Authors: Placco, Vinicius M. (Author), Beers, Timothy C. (Author), Ivans, Inese I. (Author), Filler, Dan (Author), Imig, Julie A. (Author), Roederer, Ian U. (Author), Abate, Carlo (Author), Hansen, Terese (Author), Cowan, John J. (Author), Lawler, James E. (Author), Schatz, Hendrik (Author), Sneden, Christopher (Author), Sobeck, Jennifer S. (Author), Aoki, Wako (Author), Smith, Verne V. (Author), Bolte, Michael (Author), Frebel, Anna L. (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2016-01-07T17:31:41Z.
Subjects:
Online Access:Get fulltext