The Century Survey Galactic Halo Project is a photometric and spectroscopic survey from which we select relatively blue stars (V-R
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The Century Survey Galactic Halo Project. I. Stellar Spectral AnalysisBrown, Warren R. et al.92003
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The Century Survey Galactic Halo Project. II. Global Properties and the Luminosity Function of Field Blue Horizontal Branch Stars
We discuss a 175 deg2 spectroscopic survey for blue horizontal branch (BHB) stars in the Galactic halo. We use the Two Micron All Sky Survey (2MASS) and the Sloan Digital Sky Survey (SDSS) to select BHB candidates, and we find that the 2MASS and SDSS color selection is 38% and 50% efficient, respectively, for BHB stars. Our samples include one
Brown, Warren R. et al.Advertised on:
92005 -
The chemical composition of the Orion star forming region: stars, gas, and dust
Not Available
Simón-Díaz, S.Advertised on:
92009 -
The chemical composition of the post-asymptotic giant branch F supergiant CRL 2688
We present an analysis of a high-resolution (R ˜ 50 000) optical spectrum of the central region of the protoplanetary nebula CRL 2688. This object is thought to have recently moved off the asymptotic giant branch (AGB) and displays abundance patterns of CNO and heavy elements that can provide us with important clues to help us understand the
Ishigaki, Miho N. et al.Advertised on:
92012 -
The Chemical Enrichment History of the Small Magellanic Cloud and its Gradients
We present stellar metallicities derived from Ca II triplet spectroscopy in over 350 red giant branch stars in 13 fields distributed in different positions in the Small Magellanic Cloud, ranging from ~1° to ~4° from its center. In the innermost fields, the average metallicity is [Fe/H] ~-1. This value decreases when we move away toward outermost
Carrera, Ricardo et al.Advertised on:
92008 -
The Chemical Evolution of the Monoceros Ring/Galactic Anticenter Stellar Structure
The origin of the Galactic Anticenter Stellar Structure (GASS) or "Monoceros Ring"—a low-latitude overdensity at the edge of the Galactic disk spanning at least the second and third Galactic quadrants—remains controversial. Models for the origin of GASS generally fall into scenarios where either it is a part (e.g., warp) of the Galactic disk or it
Chou, Mei-Yin et al.Advertised on:
92010