PDF-1 ASTROPHYSICAL JETS AND OUTFLOWS Elisabete M. de Gouveia Dal Pino I

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2 show a chain of more or less regularly spaced emission knots which in some cases move at high speeds away from the central source iv often terminate in emission

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1 ASTROPHYSICAL JETS AND OUTFLOWS Elisabete M. de Gouveia Dal Pino I: Transcript

2 show a chain of more or less regularly spaced emission knots which in some cases move at high speeds away from the central source iv often terminate in emission lobes with line emission in the c. Molecular Outflows in Low- and High-MassStar-forming RegionsH 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. Primordial. or . Astrophysical. ?. Jungyeon. Cho. Chungnam. National . University, Korea. Cho & . Yoo. (2012; . ApJ. ). Cho (2013; PRD). Cho (2014, . ApJ. ). Origin of Magnetic fields in the ICM. : 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. Yuri . Lyubarsky. Ben-Gurion University. Beer-. Sheva. , Israel . Universality of . relativistic jets. M 87. M 87. Crab in X-rays. GRBs. t. ime, s. t. ime, s. PKS 2155-304 . Pulsar magnetosphere. 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. . 2 show a chain of more or less regularly spaced emission knots which in some cases move at high speeds away from the central source; (iv) often terminate in emission lobes (with line emission in the c Jonathan Carroll-Nellenback. Center for Integrated Research Computing. University of Rochester. Turbulence Workshop. August 4. th. 2015. Talk Outline. . Introduction to Turbulence in the context of gaseous flows. 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. protostellar. cores?. Chat Hull. University of California, Berkeley (USA). Radio Astronomy Laboratory. 5. February 2013. Session: Magnetic Fields in the ISM and Star-forming Regions I. Magnetic Fields in the Universe IV. 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. MORNING BUSINESS Mr MCCONNELL Mr President I ask unanimous consent that the Sen-ate proceed to legislative session for a period of morning business with Sen-ators permitted to speak therein for up to 1GILBERT PINOFROM ANY POSITION OF EMPLOYMENT MANAGEMENT OR CONTROL OF ANY ESCROW AGENT123456789101112131415161718192021232425262728State of California Department of Business OversightMARY ANN SMITH De Seyfert. Galaxies Ark 564 and . Mrk. 590. Anjali. Gupta. Columbus State . Ohio State University. Collaborators: . Smita. . Mathur. , . Yair. . Krongold. Low velocity outflows are ubiquitous. .

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