Stellar models, globular and open clusters, satellite dwarfs: all are tracers of the chemical and dynamical evolution of the MW and LG galaxies

TOSI, MonicaMonicaTOSIBELLAZZINI, MicheleMicheleBELLAZZINIBRAGAGLIA, AngelaAngelaBRAGAGLIACARRETTA, EugenioEugenioCARRETTACASSISI, SantiSantiCASSISICurir, A.A.CurirLUCATELLO, SaraSaraLUCATELLOMAGRINI, LAURALAURAMAGRINIRANDICH, Maria SofiaMaria SofiaRANDICHROMANO, DonatellaDonatellaROMANOSPAGNA, AlessandroAlessandroSPAGNAVENTURA, PaoloPaoloVENTURAANNIBALI, FRANCESCAFRANCESCAANNIBALISOLLIMA, ANTONIO LUIGIANTONIO LUIGISOLLIMARe Fiorenti, P.P.Re Fiorenti2020-07-032020-07-032015http://hdl.handle.net/20.500.12386/26303ELETTRONICOenStellar models, globular and open clusters, satellite dwarfs: all are tracers of the chemical and dynamical evolution of the MW and LG galaxiesMultimediahttp://www.sexten-cfa.eu/images/stories/conferenze2015/ChemDinEvo15/Chemical_evolution_2015.htm2015cdem.confE..18TFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation