Everything you always wanted to know about stars… Material from Chapters 8 and 9 in Horizons by Seeds 0.
1/9/2003Ringberg Workshop1 Recent science results from VLTI commissioning Francesco Paresce European Southern Observatory.
T Tauri Stars Kate Barnes A540. T Tauri Stars: Background Very young, solar-type stars ~10 7 yrs Low mass 0.5 M < M < 2 M Name: T Tauri, found in Taurus-Auriga.
O. Absil & C. Eiroa with inputs from A. Roberge, D. Defrère, C. Beichman, W. Danchi, J.-C. Augereau, etc. O. Absil & C. Eiroa with inputs from A. Roberge,
Christian Knigge University of Southampton School of Physics & Astronoy Cataclysmic Variables: 10 Breakthroughs in 10 Years P. Marenfeld and NOAO/AURA/NSF.
SPECTROSCOPY OVERVIEW The Science Case: High Resolution Spectroscopy of (cool) stars Basic tools for specifications and verification One example of similar.
1 Some key problems and key reactions in Nuclear Astrophysics Main issues: BBN: was the universe always the same? What’s in the core of Sun and other MS.
The Effects of Mass Loss on the Evolution of Chemical Abundances in Fm Stars Mathieu Vick 1,2 Georges Michaud 1 (1)Département de physique, Université.
The Family of Stars Chapter 8:. Organizing the Family of Stars: The Hertzsprung-Russell Diagram We know: Stars have different temperatures, different.
Star Clusters
Characterising exoplanetary systems with space-based Bracewell interferometers ARC meeting Denis Defrère Liege, 19 February 2009.
Photometric detection of the starlight reflection by a “Pegasi” planet Martin Vannier (1), Tristan Guillot (2), Suzanne Aigrain (1) (1) ESO, Chile (2)
