Dark Matter and the Structure of the Universe Jaan Einasto Tartu Observatory 04 October 2007.
What stellar properties can be learnt from planetary transits Adriana Válio Roque da Silva CRAAM/Mackenzie.
References: Sozzetti, A., et al. 2007, ApJ, 664, 1190 Mandushev, G., et al. 2007, ApJ, 667, L195 Sozzetti, A., et al. 2007a, ApJ, in preparation Sozzetti,
A Simple Prescription for Envelope Binding Energy
HR Diagrams
APOGEE: The Apache Point Observatory Galactic Evolution Experiment l M. P. Ruffoni 1, J. C. Pickering 1, E. Den Hartog 2, G. Nave 3, J. Lawler 2, C. Allende-Prieto.
HR Diagrams AST 112. Measurements We can measure: – Temperature – Mass – Spectra – Size – Luminosity – Distance We can make measurements on trillions.
A Search for Earth-size Planets Borucki – Page 1 Roger Hunter (Ames Research Center) & Kepler Team March 26, 2010.
Nuclear Incompressibility and Compact Stars Fridolin Weber, San Diego State University.
The power plant of the Sun and stars. Nuclear Reactions in Stellar Interiors H + H 2 H + e + + nu H + 2 H 3 He + gamma 3 He + 3 He 4 He + H + H Net effect:
Leslie Rogers Hubble Fellow California Institute of Technology [email protected] Kepler Science Conference II – November 4, 2013 Glimpsing the Compositions.
ihorn To see a world in a grain of sand… Michael R. Meyer Institute for Astronomy, ETH-Zurich Dynamics of Discs and Planets Isaac Newton Institute.
