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Table · dataset · 2010

Spectroscopic study of Leo V dSph

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We present a spectroscopic study of Leo V, a recently discovered satellite of the Milky Way (MW).

Description

From stellar spectra obtained with the MMT/Hectochelle spectrograph we identify seven likely members of Leo V. Five cluster near the Leo V center (R<3') and have a velocity dispersion of 2.4^+2.4^_1.4_km/s. The other two likely members lie near each other but far from the center (R~13'~700pc) and inflate the global velocity dispersion to 3.7^+2.3^_1.4_km/s.

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Astronomical sciences 72%
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