The Universe Tonight, May 7, 2011
Characterizing exoplanets atmospheres and surfaces Thérèse Encrenaz LESIA, Observatoire de Paris Pathways Toward Habitable Planets Barcelona, 14-18 September.
Stellar Physics 10 lectures, exploring the development of cosmology, and some of the key ideas of Big Bang theory Access PPT slides at .
Eso1148
Application of X-ray plasma diagnostics to nova winds
NASA FISO Presentation: Lunar Flashlight: Mapping Lunar Polar Volatiles Using a Cubesat
White Dwarfs With contributions from S. R. Kulkarni T. Monroe.
High Contrast AO Imaging at the MMT with ARIES SDI Laird Close, Beth Biller, Eric Nielsen Don McCarthy & MMT AO Group (Steward Obs)
Star Properties. Apparent Magnitude System of Hipparchus Group of brightest stars1 m Stars about ½ as bright as 1 m 2 m Stars about ½ as bright as 2 m.
The Properties of Young Brown Dwarfs John D. Shaw.
Most Stars Are Single ! C. J. Lada ApJ, 640, L63 (2006) 1.From observations: a low binary fraction for late-type stars 2.2/3 of all disk MS stellar systems.
JENAM-2011, SpS3 Oleg Malkov, Olga Dluzhnevskaya, Sergey Karpov, Elena Kilpio, Aleksey Kniazev, Aleksey Mironov, Sergey Sichevskij Institute of Astronomy,
