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1. stAAS Winter Meeting Abstracts90 – HAD I Special: Making Astronomy Public, Los Astrophysics with CCAT in the Next Decade243 – Galaxy ClustersAngeles Style 151 –…
Slide 1Duilia de Mello (CUA-GSFC) Amy Soto (CUA), Nick Bond (GSFC), Jon P. Gardner (GSFC), Swara Ravindranath (STScI), Claudia Scarlata (UMN), Elysse Voyer (LAM), Harry Teplitz…
Slide 1What can emission lines tell us? lecture 1 Grażyna Stasińska Slide 2 Slide 3 some basic literature dealing with the ionized ISM books Physical Processes in the Interstellar…
Slide 1Protostars are difficult to observe because A. the protostar stage is very short. B. they are surrounded by cocoons of gas and dust. C. they radiate mainly in the…
1. The Magnetic Field of the Irregular Galaxy NGC 4214Amanda A. Kepley1 , Ellen G. Zweibel, Eric M. Wilcots Washburn Observatory, University of Wisconsin, 475 North Charter…
3D-PDR: A new three-dimensional radiative transfer and astrochemistry code for treating Photodissociation Regions With thanks to “Friends for Astronomy Group”, Thessaloniki…
1. NEBULA Anebulais aninterstellar cloudofdust ,hydrogengas andplasma . It is the first stage of astar 's cycle. 2. BOOMERANG NEBULA Originallynebulawas a general name…
Slide 1 27/09/06 D. Fenech Jodrell Bank Observatory Supernova Remnants in the Central Starburst Region of M82 EVN Symposium 2006 Slide 2 27/09/06 D. Fenech Jodrell Bank Observatory…