PPT-Studying Parsec Scale Jets

Author : luanne-stotts | Published Date : 2016-06-13

in Star Forming Region Tae Soo Pyo Subaru Telescope NearIR NBFs Survey of Jets in Massive Star Forming Region with GLAO Key words GLAO FWHM 02 FoV 15x 15

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Studying Parsec Scale Jets: Transcript


in Star Forming Region Tae Soo Pyo Subaru Telescope NearIR NBFs Survey of Jets in Massive Star Forming Region with GLAO Key words GLAO FWHM 02 FoV 15x 15 . 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. G. Heinrich, J. . Huston. , J. . Maestre. , D. . Maitre. , R. . . Pittau. ,. G. . Soyez. (jet . liason. ). Understanding cross sections at the LHC. PDF. ’. s, PDF luminosities. and PDF uncertainties. : 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. This triangle should be 4,500 times longer!. d . (distance to star) . is in parsec units . 1 parsec = 206,265 . x. 1 A.U.. ab. . (distance Earth to Sun) . has to be in Astronomical Units (A.U.). p. : Parallel Runtime Scheduling and Execution Controller. Jack . Dongarra. , George . Bosilca. , . Aurelien. . Bouteiller. , Anthony . Danalis. , Mathieu . Faverge. , . Thomas Herault. Also thanks to: . 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. . Tutorial Contents Part 1: Understanding PARSEC OverviewHistory, Impact, What’s NewWorkloadsResearch on PARSEC Part Working with PARSEC The parsecmgmttoolBuilding & Running workloadsConfiguration Suite PARSEC 3.0 ARCO Group seminar 27th January of 2012 Mart ggF. ->Higgs(+jets). J. Huston, S. Ellis, B. . Mellado. Scale uncertainty. The Higgs cross section depends on the renormalization scale . m. R. and factorization scale . m. F. Consider default values for these two scales, . 12345678 12345678 LinearBodytrack (PARSEC 1.0)Bodytrack (PARSEC 2.0)Number of CoresSpeedup Figure1:ComparisonofthespeedupsofthebodytrackworkloadsofPARSEC1.0and2.0.Theimprovedparalleliza-tionachieves30 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. …some points for discussion. J. Huston. Michigan State University. 1. Start with Stewart-. Tackmann. c. learly, scale uncertainty for. e. xclusive cross sections . d. on’t vanish, so naïve scale. 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. Night sky rule of thumb. :. one finger width = 2 deg. . one hand width = 10 deg.. Units for Time and Distance. Kilometer (km). = .621 miles. Light-year (. lt-yr. ). = The distance light travels in one year in a vacuum. .

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