skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: A search for stars of very low metal abundance. VI. Detailed abundances of 313 metal-poor stars

Journal Article · · Astronomical Journal (New York, N.Y. Online)
; ; ; ; ;  [1];  [2]
  1. Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)
  2. Department of Astronomy, University of Texas at Austin, 1 University Station, C1400, Austin, TX 78712 (United States)

We present radial velocities, equivalent widths, model atmosphere parameters, and abundances or upper limits for 53 species of 48 elements derived from high resolution optical spectroscopy of 313 metal-poor stars. A majority of these stars were selected from the metal-poor candidates of the HK Survey of Beers, Preston, and Shectman. We derive detailed abundances for 61% of these stars for the first time. Spectra were obtained during a 10 yr observing campaign using the Magellan Inamori Kyocera Echelle spectrograph on the Magellan Telescopes at Las Campanas Observatory, the Robert G. Tull Coudé Spectrograph on the Harlan J. Smith Telescope at McDonald Observatory, and the High Resolution Spectrograph on the Hobby-Eberly Telescope at McDonald Observatory. We perform a standard LTE abundance analysis using MARCS model atmospheres, and we apply line-by-line statistical corrections to minimize systematic abundance differences arising when different sets of lines are available for analysis. We identify several abundance correlations with effective temperature. A comparison with previous abundance analyses reveals significant differences in stellar parameters, which we investigate in detail. Our metallicities are, on average, lower by ≈0.25 dex for red giants and ≈0.04 dex for subgiants. Our sample contains 19 stars with [Fe/H] ≤–3.5, 84 stars with [Fe/H] ≤–3.0, and 210 stars with [Fe/H] ≤–2.5. Detailed abundances are presented here or elsewhere for 91% of the 209 stars with [Fe/H] ≤–2.5 as estimated from medium resolution spectroscopy by Beers, Preston, and Shectman. We will discuss the interpretation of these abundances in subsequent papers.

OSTI ID:
22340236
Journal Information:
Astronomical Journal (New York, N.Y. Online), Vol. 147, Issue 6; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1538-3881
Country of Publication:
United States
Language:
English

Similar Records

CHARACTERIZING THE CHEMISTRY OF THE MILKY WAY STELLAR HALO: DETAILED CHEMICAL ANALYSIS OF A METAL-POOR STELLAR STREAM ,
Journal Article · Wed Mar 10 00:00:00 EST 2010 · Astrophysical Journal · OSTI ID:22340236

A NEW ABUNDANCE SCALE FOR THE GLOBULAR CLUSTER 47 Tuc
Journal Article · Tue Apr 15 00:00:00 EDT 2008 · Astronomical Journal (New York, N.Y. Online) · OSTI ID:22340236

A DIFFERENTIAL CHEMICAL ABUNDANCE SCALE FOR THE GLOBULAR CLUSTER M5
Journal Article · Tue Jun 15 00:00:00 EDT 2010 · Astronomical Journal (New York, N.Y. Online) · OSTI ID:22340236