Star & Planet Formation Minicourse, U of T Astronomy Dept. Lecture 5 - Ed Thommes Accretion of Planets Bill Hartmann.
N.36 turrini jupiter-and-the-early-collisional-evolution-of
O. Mousis (UTINAM, Université de Franche-Comté, France) L. N. Fletcher (Oxford U., UK), N. André (IRAP, France), M. Blanc (IRAP, France), A. Coustenis.
Low-mass H-burning stars, brown dwarfs, & planets 13 M J 80 M J Planets Mayor & Queloz 1995 Brown dwarfs Rebolo et al. 1995 Stars 1 M J = 0.01 M
Exo-planets: ground-based How common are giant planets? What is the distribution of their orbits? –3.6m HARPS: long-term radial velocity monitoring of.
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,
D. Turrini 1, M. Barbieri 2, F. Altieri 1, D. Grassi 1, A. Adriani 1, G. Piccioni 1 1 Institute for Space Astrophysics and Planetology INAF-IAPS 2 Center.
JUPITER AARON AND EDWARD JUPITER is the biggest planet of all the other planet. JUPITER is the fifth planet away from the sun.
Blue Dots Workshop in Paris, Nov 17/18, 2008 Key Questions in Planet Formation and Evolution
PHYS178 2008 week 11 part-1
1 High Contrast Imaging Extreme AO & 30-m Telescopes James R. Graham UC Berkeley 2005/02/16.
Ge/Ay133
