PPT-Jets in Flight

Science Topic Physics Designing a Navy Jet Fighter Lesson Objectives Understand the Engineering Design Process Comprehend the basic principles of flight Apply the Engineering Design Process to aircraft design. brPage 1br JETS eia K Tun K ckkf K chc ch jK xR Ksvs KT Ksz Ks K RwuSvwRsT K K Tz KsTwvUVs KsTRsRuzS K syw SK K K zsRRS VK Th K narrativ K materia Ko Kye K gle ed Kwhic K catalogue K th Kage Ko Ramesh Narayan. Jets are Widespread. Relativistic Jets . occur widely in . accreting black holes (BHs): AGN, XRBs, GRBs. A . common . robust . mechanism . must be producing all these . Jets. Best Bet. Gamma ray bursts (GRB) are an especially exciting outflow phenomena that are capable of outputting as much energy as our sun will. Christopher C. . Lindner. 1. Abstract. Relativistic Jets are streams of plasma moving throughout the universe at speeds up to 99% the speed of light. They produce high-energy X-ray, radio, and visible radiation that are observable from great distances across the universe. flavor . produced in association with W and Z bosons. Pierre-Hugues Beauchemin. o. n behalf of the ATLAS Collaboration. Tufts University. ICHEP2012 -Melbourne, Australia . 0. 5/07/2012. Outline. Context of the measurements. The View From Telescopes, Computers. and the Lab. Adam Frank. University of Rochester. A Cast Of Lots and Lots. AstroBEAR development. : J. Carroll, B. . Lui. , M. . Huarte. -Espinosa, S. Li, E. Hanson, E. Kaminski, K. . : data . vs. theory. Joey Huston. Bruce . Mellado. 1. Higgs(->. gg. )+jets. Most of the excess observed for Higgs production is in >=1 jet final states. Maybe CMS does not see as large of an excess. Squarks. and . Gluinos. in the Jets + MET + 0-Lepton Channel at ATLAS. Dan . Tovey. University of . Sheffield. On behalf of the ATLAS Collaboration. 2. The ATLAS Detector. Inner Detector (|. . |<2.5, B=2T): . in Star Forming Region. Tae-. Soo. . Pyo. Subaru Telescope. Near-IR . NBFs. Survey of Jets in Massive Star Forming Region with GLAO. . Key words:. -. GLAO : FWHM ~ 0.2” , . FoV. ~ 15’x 15’. . Circinus. X-1 with Very Long Baseline . Interferometry. James Miller-Jones. Collaborators: A. . Moin. , S. . Tingay. , C. Reynolds, C. Phillips, . A. . Tzioumis. , R. Fender, J. McCallum, G. Nicolson, V. . Squarks. and . Gluinos. in the Jets + MET + 0-Lepton Channel at ATLAS. Dan . Tovey. University of . Sheffield. On behalf of the ATLAS Collaboration. 2. The ATLAS Detector. Inner Detector (|. . |<2.5, B=2T): . Tsvi Piran. Racah. Institute of Physics,. The Hebrew University. Omer Bromberg, Ehud . Nakar. Re’em. Sari. , . Franck Genet, Martin . Obergaulinger. , Eli . Livne. T Piran Jets 2011 Krakow . The (long) GRB-Supernova connection. A . Middle-aged Pulsar's New Trick. Q. . Daniel . Wang & Seth Johnson . University . of . Massachusetts. B2224+. 65 . and . Guitar. . Nebula. Period = 0.68 s. Ė. s. . =1.2 x 10. 33. erg s. −1. Theory. Mario Livio. Space Telescope Science Institute. Which Systems Have Highly Collimated . Jets. ?. Object . Physical System. Young Stellar Objects. Accreting Star. HMXBs. Accreting NS or BH. X-ray Transients. W - � enu varsha ramakrishnan Double parton scattering 2 RAW JETS FROM THE NUTPLE REMOVE “Electron JETS” APPLY JET ENERGY SCALE CORRECTION L5 SELECT JETS WITH E T �12 GeV /|