The 300 km s -1 stellar stream near Segue 1: Insights from high-resolution spectroscopy of its brightest star
We present a chemical abundance analysis of 300S-1, the brightest likely member star of the 300 km s-1 stream near the faint satellite galaxy Segue 1. From a high-resolution Magellan/MIKE spectrum, we determine a metallicity of [Fe/H] = -1.46 ± 0.05 ± 0
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Frebel_The_300_km_s_-1__stellar_2013.pdf||1.35 MB||Adobe PDF||Request a copy|
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