The intringuing hot molecular core G31.41+0.31. Maite Beltrán Osservatorio Astrofisico di Arcetri. The HMC G31.41+0.31. UC HII. Clump. HMC. G31.41 is located at a distance of 7.9 kpc, L IRAS = 3x10 5 L ➔ consistent with an embedded star of 25 M .By nemo
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BIZ JETS!! BIZ JETS!! BIZ JETS!! BIZ JETS!! BIZ JETS!!. BIZ JETS!!. Canadair CL-600 Challenger Canadair CL-601 Challenger Canadair CL-604 Challenger Canadair CL-800 Challenger Bombardier BD-100 Challenger 300 Bombardier BD-700 Global Express Rockwell 1121 Jet Commander
Jets. Two classes of jets from X-ray binaries Jet power versus accretion power Jet composition Large-scale jets and interactions with ISM Jet production and collimation. Two Flavors of Radio Jets. Compact – tens of AU, found in low/hard X-ray state.
First Jet Results using the Upgraded D0 Detector Nirmalya Parua (for the D0 Collaboration) State University of New York Stony Brook DPF 2002 College of William and Mary Williamsburg, Virginia, May 24-28, 2002. Jets. Jet is a collection of towers within a given cone R.
Ofek Birnholtz, Tsvi Piran Racah Institute of Physics, Hebrew University of Jerusalem arXiv:1302.5713v2 , submitted to PRD Yukawa International Seminar Yukawa Institute for Theoretical Physics Kyoto, Japan, 3.6.2013. GW Memory from GRB Jets a possible DECIGO source.
Jets. Come to the end zone and learn all about the best team in NFL!. Presented by: Helen Fahey Project 12: My Favorite Sports Team January 9, 2012. Background Information on The Jets.
JETS. How are jets observed? How do they interact with their surroundings? The radiation from jets Where do they come from? Tracing them to their source How are they made? Magnetic propulsion Energy source? Accretion or BH spin?. Cygnus A VLA, 21-cm radio emission. RADIO GALAXIES.
CCHS JETS. “Take off with School Wide Positive Behavior Support!”. Our Team. Our team is made up of teachers, administrators, guidance, and students We take input from many different angles to allow the program to fit everyone. Our Beginnings. Pre-meeting's to set goals (brain storming)
W+ Jets. Varsha Ramakrishnan UW Madison HEP Group meeting 03/30/09. Outline of the Talk. Jet Selection Cuts “Electron-Jet Removal” Properties of all Jets after “Electron-Jet” Removal Leading Jet and Next-to Leading Jet variable distributions Look at Next-to-Next Leading Jet properties