[Distillation] - Towers Malfunctions (Kister)
How a Well Flows
Large-scale components of radio galaxies in gamma rays Martin Hardcastle Heidelberg, Gamma2012 Thanks: Judith Croston, Teddy Cheung, Łukasz Stawarz.
Hour 2: Stars, Stellar Evolution, and Creation of Chemical Elements The Sun & Nuclear Fusion - Energy for Life The Sun Compared With Other Stars Stellar.
Validation of local gravity Mr. Neville Tayler South African National Accreditation System.
Stellar Evolution: Parts of Chapters 12,13,15,16 Stellar Evolution: Parts of Chapters 12,13,15,16 Stars lose energy - hence they must evolve. Stars lose.
Simulations of Emerging Magnetic Flux in Active Regions W. P. Abbett Space Sciences Laboratory University of California, Berkeley.
Plasma Physics in the Solar System Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics.
1 ESS200C Planetary Ionospheres Lecture 16. 2 Interactions with the Moon The Moon has no significant atmosphere and no ionosphere. The lunar crust is.
Plasma in the Heliosheath John Richardson M.I.T. Collaborators: J. Belcher, J. Kasper, E. Stone, C. Wang.
1 Enrique Vázquez-Semadeni Adriana Gazol CRyA UNAM, México Collaborators: Thierry Passot (OCA) Jongsoo Kim (KASI) Dongsu Ryu (Chungnam U.) Ricardo González.
Atomic and Molecular Gas in Galaxies Mark Krumholz UC Santa Cruz The EVLA: Galaxies Through Cosmic Time December 18, 2008 Collaborators: Sara Ellison (U.