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Towards the science case for E-ELT HIRES – Cambridge, Sept 13-14, 2012

Towards the science case for E-ELT HIRES – Cambridge, Sept 13-14, 2012. E-ELT HIRES SCIENCE CASES: STELLAR SPECTROSCOPY and YOUNG STARS. optical+near IR high res stellar spectroscopy. 8-10m class telescopes massive stars, luminous giants/SGs in the Galaxy & LG. PMS. E-ELT

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Towards the science case for E-ELT HIRES – Cambridge, Sept 13-14, 2012

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  1. Towards the science case for E-ELT HIRES – Cambridge, Sept 13-14, 2012 E-ELT HIRES SCIENCE CASES: STELLAR SPECTROSCOPY and YOUNG STARS optical+near IR high res stellar spectroscopy 8-10m class telescopes massive stars, luminous giants/SGs in the Galaxy & LG PMS E-ELT low luminosity stars in the Galaxy luminous stars in the LG and beyond Livia Origlia – INAF Bologna, Italy

  2. Towards the science case for E-ELT HIRES – Cambridge, Sept 13-14, 2012 E-ELT HIRES SCIENCE CASES: STELLAR SPECTROSCOPY and YOUNG STARS optical + near IR high res stellar spectroscopy @ E-ELT stellar populations (Tolstoy & de Laverny talks) chemical evolution & stellar archaeology stellar physics, evolution & nucleosynthesis young stars (Testi/Nisini) proto-star & star-disk interaction  planet formation distant star clusters (Larsen talk) chemical composition & dynamical mass constraints on the IMF & the host galaxy Livia Origlia – INAF Bologna, Italy

  3. Towards the science case for E-ELT HIRES – Cambridge, Sept 13-14, 2012 E-ELT HIRES SCIENCE CASES: STELLAR SPECTROSCOPY and YOUNG STARS optical + near IR high res stellar spectroscopy @ E-ELT very high s/n … very precise chemical abundances (Gustafsson & Korn talk) very precise stellar parameters (Ammler-von Eiff, Tautenburg) isotopic abundances (Israelian talk + 12C18O,12C17O 2.349-2.352 mm R>=100k) granulation in stars with transiting planets (Dravins – Lund) = - high resolution line profiles across spatially resolved stellar disks! asteroseismology in M dwarfs (Gonzalez & Rodriguez-Lopez - Granada) pulsations will help determining the frontier between partially- and fully-convective structure in M dwarfs (SpT M3.5 ?) Livia Origlia – INAF Bologna, Italy

  4. Towards the science case for E-ELT HIRES – Cambridge, Sept 13-14, 2012 E-ELT HIRES SCIENCE CASES: STELLAR SPECTROSCOPY and YOUNG STARS top level requirements spectral range: 0.310.38 - 2.4 micron Be 3130 AA R>50,000 OH UV lines NH 3360 AA Balmer jump ~3600 AA U II 3859 AA CN 3883 AA HF 2.336 mm R>50,000 12C18O,12C17O 2.349-2.352 mm R>=100,000 spectral resolution: R~20k  R~100K  1medium, 1high spectral sampling: > 2 pix RV accuracy:m/s (stellar oscillations) • observing modes/feeding: mostly point sources • fibers desirable for highly accurate measures (e.g. RV, line profiles etc.) • some MOS capability desirable for stellar pop studies • desirable spatially resolved slit/IFU for CS disks/jets Livia Origlia – INAF Bologna, Italy

  5. Calibration: blaze effects very high resolution: 300k

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