Physics
Scientific paper
Jul 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011eas....48..215z&link_type=abstract
EAS Publications Series, Volume 48, 2011, pp.215-216
Physics
Scientific paper
The Phoenix dwarf galaxy is the nearest and most typical representative of the class of the so-called transition dwarf galaxies (from spheroidal to irregular). We present here precise velocity measurements obtained from high-resolution spectroscopy of more than one hundred member stars, allowing us to study the stellar kinematics and estimate the internal velocity dispersion and dark matter content.
Held Enrico V.
Momany Yazan
Rizzi Luca
Saviane Ivo
Sommariva Veronica
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