Multi-object spectroscopy of massive stars in the Local Group and beyond

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40Telescope developmentDiametermirror (m)E-ELT105VLT01600 1700 1800 1900 2000 2100
Extremely Large Telescope
Page 1 and 2: Multi-object spectroscopy of massiv
Page 3 and 4: Key questions to be addressed• Ho
Page 5 and 6: Crowther et al. (2010)
Page 7 and 8: Evidence for stars with M init > 15
Page 9 and 10: Bohannan & Conti 1976, ApJ 204, 797
Page 11 and 12: How to make a massive star?(a) A de
Page 13: Very Large Telescope, Cerro Paranal
Page 16 and 17: Central star powering UCHIIIonizing
Page 18 and 19: Massive YSOs in RCW36Ellerbroek et
Page 20 and 21: Mass loss and accretion diagnostics
Page 22 and 23: Massive stars are born as giants: B
Page 24 and 25: SED B275:SpType B0 VL ~ 20,000 Lod
Page 26 and 27: VLT/X-shooter spectrum M17-B275Ochs
Page 28 and 29: B275: “bloated” PMS star contra
Page 30: VLT/FLAMES Tarantula Survey(Evans e
Page 33 and 34: Triggered star formation by 30 Dor
Page 35 and 36: Tramper et al. 2011, ApJ 741, L8
Page 37 and 38: First VLT/X-shooter spectrum of mas
Page 39: Obtaining spectra of O stars in Loc
Page 43 and 44: Chapman et al. (2006)Richardson et
Page 45 and 46: ANGST SurveyDalcanton et al. (2009)
Page 48 and 49: E-ELT MOS• Explore E-ELT’s larg
Page 50 and 51: RSG J-band spectra in Virgowith S/N
Page 52 and 53: ➡ E-ELT: galaxies out to 35Mpc (m
Page 54 and 55: Conclusions• With the E-ELT it wi

Multi-object spectroscopy of massive stars in the Local Group and beyond

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