IAU Symp. 276, Torino, october 2010 R. Gratton 1, M. Kasper 2, C. Verinaud 3, M. Bonavita 1,4 + EPICS Science team Science with EPICS The E-ELT Planet.
Courtesy Jason Harris, Steward Observatory Two Tails of a Distribution : The Initial Mass Functions of Extreme Star Formation Michael R. Meyer Steward.
High-resolution X-ray spectroscopy of CTTS and WTTS reveals an anomaly among CTTS: The observed OVII r /OVIII Ly is large in CTTS (of order unity) whereas.
Extra Solar Planets ASTR 1420 Lecture 17 Sections 11.2.
Hertzsprung Russell (HR) Diagram Spectral Types: Proxy for T eff Or surface temperature
Two Tails of a Distribution : The Initial Mass Functions of Extreme Star Formation
X-ray and observational Astronomy
X-ray and observational Astronomy Detection limits for close eclipsing and transiting sub- stellar and planetary companions to white dwarfs in the WASP.
“Where to Study Planet Formation? The Nearest, Youngest Stars”
