A possible formation scenario for dwarf spheroidal galaxies - I. Fiducial model

We perform numerical simulations to study a formation scenario for dwarf spheroidal (dSph) galaxies in which their stellar populations are the products of the dissolution of open star clusters and stellar associations within cosmological dark matter haloes. This paper shows that this process gives r...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2013-06, Vol.432 (1), p.274-284
Hauptverfasser:	Assmann, P., Fellhauer, M., Wilkinson, M. I., Smith, R.
Format:	Artikel
Sprache:	eng
Schlagworte:	Cosmology Dark matter Kinematics Milky Way Satellites Star & galaxy formation
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