The 300 km s -1 stellar stream near Segue 1: Insights from high-resolution spectroscopy of its brightest star
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Frebel, Anna
Lunnan, Ragnhild
Casey, Andrew
Norris, John
Wyse, Rosemary F G
Gilmore, Gerard
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IOP Publishing
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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
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Astrophysical Journal, The
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2037-12-31
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