D EBRIS DISKS WITH H ERSCHEL : AN OVERVIEW OF THE DUNES MODELING ACTIVITIES Jean-Charles Augereau, Steve Ertel, Alexander Krivov, Jérémy Lebreton, Torsten.
Paris - Apr29, 2005Reynald Pain 1998-2003 : Concordance model Today’s question : Cosmological Constant, Vacuum Energy or Dark Energy ? SNe Ia prefer.
The Influence of Radiative Transfer on SPH Simulations of Star Formation Stuart C. Whitehouse and Matthew R. Bate E-mail: [email protected], [email protected].
Benedetta Ciardi MPA Reionization Nucleosynthesis ‘Dark Ages’ Big Bang Fluctuations begin to condense into first stars and protogalaxies Decoupling matter-radiation.
TEMPO & GOES-R synergy update and GEO-TASO aerosol retrieval for TEMPO Jun Wang Xiaoguang Xu, Shouguo Ding, Cui Ge University of Nebraska-Lincoln Robert.
The Influence of Radiative Transfer on SPH Simulations of Star Formation
Photoionisation of Supernova Driven, Turbulent, MHD Simulations of the Diffuse Ionised Gas
Surface reflectance over Land
