The main aim of the STREGA@VST survey is to unveil the Halo formation mechanism by investigating the Southern part of the Fornax stream. It will use RR Lyrae stars, LPVs and Turn-Off stars as tracers to test the presence of extended halos (extra tidal) around Fornax and Sculptor dSphS. Here we describe the current status of the this Survey.
The stellar survey STREGA@VST
M. Cignoni
2014-01-01
Abstract
The main aim of the STREGA@VST survey is to unveil the Halo formation mechanism by investigating the Southern part of the Fornax stream. It will use RR Lyrae stars, LPVs and Turn-Off stars as tracers to test the presence of extended halos (extra tidal) around Fornax and Sculptor dSphS. Here we describe the current status of the this Survey.File in questo prodotto:
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