Cambridge University Press, Proceedings of the International Astronomical Union, S317(11), p. 145-152, 2015
DOI: 10.1017/s1743921315008364
Full text: Unavailable
AbstractIn this review I will discuss the current status on determinations of the dark matter content and distribution in Milky Way dwarf spheroidals, for which the available data-sets allow the application of sophisticated mass modeling techniques.