Recent results on the evolution of Local Group dwarf galaxies obtained from VLT imaging and spectroscopy are briefly reviewed, and prospects for dwarf galaxy research at the VLT are discussed in the light of the current and forthcoming instrumentation. Som
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aDwarfgalaxiesintheLocalGroup:theVLTperspectiveEnricoV.HeldOsservatorioAstronomicodiPadova,vicolodell’Osservatorio5,35122Padova,ItalyAbstract.RecentresultsontheevolutionofLocalGroupdwarfgalaxiesobtainedfromVLTimagingandspectroscopyarebrie yreviewed,andprospectsfordwarfgalaxyresearchattheVLTarediscussedinthelightofthecurrentandforthcominginstrumentation.Someaspectsoffutureinstrumentdevelopments,suchasdeepwide- eldimagingatbothopticalandnear-infraredwavelengths,thatmaybeofadvantageforresearchontheevolutionofdwarfgalaxies,arebrie ydiscussed.1IntroductionUnderstandingtheoriginandevolutionofdwarfgalaxiesandtheirluminosityandmassdistributionsmayhaveimportantconsequencesinmodernobserva-tionalcosmology.Whiledwarfgalaxiesaredi culttostudyevenatmoderateredshifts,especiallythosewithoutactivestarformation,bothstar-formingandquiescentdwarfscanbestudiedwithconsiderabledetailintheLocalGroup(LG).DwarfgalaxiesintheLGarecloseenoughthattheprocessofstarforma-tion,theirdynamicalevolutionandtheinterplaybetweenstarsandinterstellarmediumcanbestudiedindetail.Byanalyzingtheircolor-magnitudediagramsonecanderivestarformationhistoriesandreconstructtheirevolutionatlook-backtimescomparabletotheageoftheuniverse.However,soundknowledgeoftheage-metallicityrelationisrequiredtoobtainreliabledeterminationofthestarformationhistory.Spectroscopyisthereforeneededtoaddessentialinfor-mationtoconstrainthechemicalenrichmenthistories.ThiscontributionwillfocusonstudiesofstellarpopulationsandkinematicsofresolvedLocalGroupgalaxies.Ibrie yreviewtheworkdonesofarattheVLT,anddiscusstheprospectfordwarfgalaxyresearchattheVLTinthelight
oftheexistingandforthcominginstrumentation.SomeideasforfutureVLTinstrumentsarealsopresented.
2DwarfgalaxyevolutionwiththeVLT
2.1Opticalimaging
Studiesofresolveddwarfgalaxiesinthelastdecade,usingbothHSTandgroundbasedinstrumentation,haveprovidedacomplexpictureoftheirstarformationhistories.Starformationcanproceedeitherindistinctepisodes,asinthecase
A simple and natural explanation for the dynamics and morphology of the Local Group Dwarf Spheroidal galaxies, Draco (Dra) and Ursa Minor (UMi), is ...
the Local Group or nearby galaxy clusters may have been formed as TDGs (... was reobserved with FORS2 on the ESO VLT at higher spectral resolution ...
The Sagittarius dwarf ir... 暂无评价 10页 免费 VLT Spectroscopy of RR ...dwarf galaxies in the Local Group (LG) are the dwarf spheroidals (dSphs...
the dwarf irregulars are more evenly distributed throughout the Local Group....[Vol. , on the ESO 8.2 m Kueyen telescope (VLT). Bonifacio et al....
VLT and HST observations... 暂无评价 5页 免费...Thus the existence of young dwarf galaxies in 1...the Local Group and six Local Group irregular ...
(at M_V=-10) outshining entire dwarf galaxies...Local Group galaxies, although at lower signal-to...FORS1 on the VLT (Bresolin et al. 2001, 2002...
VLT Spectroscopy of Glob... 暂无评价 18页 免费 Ultra Compact Objects in...All Local Group objects with (a-b)/a > 0.3 appear to be galaxies. ...
Hot subdwarfs in the Galactic Bulge_专业资料。...galaxies in many cases show a strong and ... of 29 EHB star candidates at the VLT-UT1 (...
dwarf stars in galaxies of the Local Group and ...The new instrument for the VLT has been named ...
Absence of Dwarf Galaxie... 暂无评价 11页 ...a galaxy cluster survey at high redshifts S. ...the VLT and the LBT (available in the course ...
dwarf and sub-luminous galaxies would be preferred...the local density of galaxies and the presence ...(VLT) at Paranal, (Chile) between March 2000 ...

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