PPT-Stars Disks and Jets

Author : myesha-ticknor | Published Date : 2016-05-15

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

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Stars Disks and Jets: Transcript


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 . 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. AS 4024 InclinationsRadial velocities give minimum masses•need inclinations– orbits–eclipsing binaries–apsidal motion 333 AS 4024 Binary Stars and Accretion Disks Astrometric Orbit : 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. 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. . a. nd stellar multiplicity. Insights from recent surveys. Gaspard . Duchêne. (UC Berkeley, Obs. Grenoble). © NASA/JPL/Caltech. Planets in multiple systems?. © . LucasFilm. Ltd.. They must exist!. 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. . 6. /27/12. In collaboration with . Avi. Loeb. Harvard University Astronomy Department. arXiv:. 1109.6660, PRL 108, 6, 061302. Observing . Lense-Thirring. Precession in Tidal Disruption Flares. Outline. M87. Studying the Cosmos through..... . Observations. Theory. Experiment. Astro @ Purdue. Astro @ Purdue. 9 . research-active faculty members covering a wide range of topics. Group includes postdoctoral scholars, staff scientists and students. Insights from recent surveys. Gaspard . Duchêne. (UC Berkeley, Obs. Grenoble). © NASA/JPL/Caltech. Planets in multiple systems?. © . LucasFilm. Ltd.. They must exist!. Planets in multiple systems!. Reads and writes are equally fast.. Arrays of these disks are used to provide highly reliable storage.. Increasingly popular as they are fast and do not contain moving parts.. Magnetic Disks.. . What is a magnetic disk and how it works. Two main types: Magnetic and Optical. Random access to memory. The hardware must be controlled by driver software called the “controller” in order to be used. Hard Disks, RAID, and Error Handling. for The Detection of ExoPlanets. C. Beichman. Friday, March 26, 2010. 5 AU Workshop . With lots of help from A. Tanner (Georgia State), G. Bryden (JPL), S. Lawler (Wesleyan/UBC), R. Akeson (NExScI), D. Ciardi (NExScI), C. Lisse (JHU), Mark Wyatt (Cambridge). 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. DRAFT VERSIOK APRIL 7, 2011 J§.'IEX style emulateapj v. 6/22/04 SPITZER IRS SPECTROSCOPY OF THE 10 MYR-OLD EF CHA DEBRIS DISK: EVIDEXCE FOR PHYLLOSILICATE-RICH IN THE TERRESTRIAL ZOXE

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