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arxiv: 1401.6372 · v1 · pith:3MML3LWUnew · submitted 2014-01-22 · 🌌 astro-ph.IM · astro-ph.GA

Stellar populations in the ELT perspective

G. Bono (1 , 2) , V. F. Braga (1) , M. Fabrizio (3) , R. Gilmozzi (4) , R. Buonanno (1 , 3) , I. Ferraro (2)
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G. Iannicola (2) M. Monelli (5) A. Milone (6) M. Nonino (7) L. Pulone (2) P.B. Stetson (8) F. Thev\'enin (9) A. R. Walker (10) ((1) Univ. Rome Tor Vergata Roma Italy (2) INAF-OAR Monte Porzio Catone (3) INAF-OATe Teramo (4) ESO Garching Germany (5) IAC La Laguna Spain (6) RSAA The Australian National University Weston Australia (7) INAF-OAT Trieste (8) DAO-HIA NRC Victoria Canada (9) Obs. C\^ote d'Azur Nice France (10) NOAO-CTIO La Serena Chile)
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classification 🌌 astro-ph.IM astro-ph.GA
keywords populationsstellaraddressastrophysicaldiscussextremelygenerationimpact
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We discuss the impact that the next generation of Extremely Large Telescopes will have on the open astrophysical problems of resolved stellar populations. In particular, we address the interplay between multiband photometry and spectroscopy.

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