PDF-magnetars, blazars, etc)

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Ct Ctdt 1cvBJBut the plasma is a very good conductor right But the plasma is a very good conductor rightRight The RHS becomes important not because collisions are

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magnetars, blazars, etc): Transcript

Ct Ctdt 1cvBJBut the plasma is a very good conductor right But the plasma is a very good conductor rightRight The RHS becomes important not because collisions are large but because sha. Magnetar. Candidate Located Outside the Galactic Plane?. Joe . Callingham. | . Sean Farrell . | Bryan . Gaensler. | Geraint Lewis. Sydney Institute for Astronomy (. SIfA. ) | The University of Sydney | Australia . distance indications from Fermi and . TeV. data: an empirical approach. E. . Prandini. , Padova University & INFN. G. . Bonnoli. , L. . Maraschi. , M. . Mariotti. and F. . Tavecchio. SciNeGHE. as Seen at . Very High Energies. Elisa Prandini . Dipartimento. . di. . Fisica. & INFN Padova. . prandini@pd.infn.it. Dipartimento. . di. . Astronomia. , . Padova, 23. rd. June 2011. Outline. Blazars. Naoki . Isobe. , Yoshihiro Ueda (Kyoto University). Kousuke. . Sugimori. , Nobuyuki Kawai (Tokyo Tech.). Hitishi. . Negoro. (Nihon Univ.). . Mutsumi. . Sugizaki. , Masaru Matsuoka (RIKEN). within the field . of Fermi unassociated gamma-ray sources. Yamaguchi . U. niv.. Yoshitaka FUJINAGA. K. . Ninuma. , A. Kimura, K. Fujisawa, K. . Akutagawa. , K. Sugiyama, K. . Motogi. . (Yamaguchi Univ.) . Alan Marscher. Institute for Astrophysical Research, Boston University. Research Web Page: www.bu.edu/blazars. Disclaimer. The data and discussion presented here are but a small subset of the huge number of both wonderful and not-so-wonderful multi-waveband studies.. Yun. -Wei YU. 俞云伟. June 22, 2010, Hong Kong. Outline. Background. Implications from the shallow decay afterglows of GRBs. A qualitative discussion on . magnetar. wind emission. Emission from the termination shock of the wind. Jun 22, 2010. HKU Fermi Workshop. Neutron Star Zoo: radio pulsars, . magnetars. , RRATs, CCOs, and more . Special thanks to Vicky . Kaspi. for some materials in this talk . Overview. Since the first pulsar discovered 40 yrs ago, they are . Joe . Callingham. | . Sean Farrell . | Bryan . Gaensler. | Geraint Lewis. Sydney Institute for Astronomy (. SIfA. ) | The University of Sydney | Australia . Image credit: NASA. A New . Magnetar. Candidate. Swift. -BAT blazars with . NICER. Sergio Mundo, Richard . Mushotzky. University of Maryland, College Park. MARLAM 9, JHU, Baltimore, MD. Blazar characteristics. Radio-loud AGN with jet aligned close to line of sight. magnetars and rotation-powered pulsars. Hongjun An. 1. and the NuSTAR Team. 1. McGill University. Launched on 2012 June 13. Focusing in the hard X-ray band (>10 keV). Two orders of magnitude better sensitivity in the 10—79 keV. Matthew Fu. 1. , Timothy Govenor. 1. , Quentin King. 1. , . Parisa Roustazadeh. 1,2. , . Markus Boettcher. 3. 1. Bishop Watterson High School, Columbus, OH, USA. 2. Columbus State Community College, Columbus, OH, USA.

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