PPT-Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebul

20131218 Speaker Yu Hsun Cheng Professor Yosuke Mizuno Introduction Supernova remnantsSNR This is the structure resulting from the explosion of a star in a supernova  It is formed by that the interactive between interstellar and . S.P. Reynolds et al.. Martin, Tseng Chao . Hsiung. 2013/12/18. Which contents I will cover…. Shell Supernova Remnants: Obliquity Dependence, and . Summary!. Magnetic Fields in Pulsar-Wind Nebulae.. Dayal Wickramasinghe and Lilia . Ferrario. Australian National University. Canberra. . . The chemically peculiar . Ap. , Bp stars ( ~ 1.8 -5 . M. sun. ) are magnetic, and . have ordered large. scale fields, . Supernova Remants and Pulsar Wind Nebulae in the Chandra Era. 1. Modeling the Dynamical and Radiative Evolution of a Pulsar Wind Nebula inside a Supernova Remnant. Joseph Gelfand (NYU / NSF). Patrick Slane (CfA), Weiqun Zhang (NYU). . 22/10/2011 INDIGO . discussions@IUCAA. . Bhal. Chandra Joshi . Radio pulsar searches . Radio pulsars - highly magnetized rotating NS - compact . - periodic pulses . http://www.cv.nrao.edu/course/astr534/Pulsars.html. http://www.nikhef.nl/pub/onderzoekschool/topics/Kuijpers1.pdf. High Energy Astrophysics. jlc@mssl.ucl.ac.uk. http://www.mssl.ucl.ac.uk/. Enrico Massaro notes. a physical perspective . . 1. Philip Judge, . . High Altitude Observatory, NCAR. "Double, double, toil and trouble;. Fire burn, and cauldron bubble!". -- . is a supernova remnant which is a super dense, . rapidly spinning neutron star which emits . dipole electromagnetic . radiation and features a strong magnetic and gravitational . field and also high space velocity. . Arunas Janusonis. CONTENT. FACTORS OF CONTAMINATION. ASSOCIATION „REMNANTS OF WAR T. H. REAT PREVENTION“. MISSION. PURPOSES. SERVICES. COOPERATION. IMPLEMENTED . PROJECTS. CONTACTS. FACTORS OF CONTAMINATION. N. eutron . Stars Foreseen. . Supernova . End Products?. When a . supernova. goes off, we can speculate that:. The star might blow itself to smithereens, . scattering all its material into space and leaving . Ingrid Stairs. UBC Vancouver. CAWONAPS. TRIUMF. Dec. 9, . 2010. Pulsars are one manifestation of neutron stars:. spin periods ~. 1.4. ms to . 8.5 seconds,. magnetic fields ~10. 8. to ~5 x10. 13. G. . all magnets have magnetic poles – . . points at the ends of a magnet that have opposing magnetic qualities. all magnets have a north pole and south pole that are magnetically opposite. like poles repel and unlike poles attract. Instrument Chemistries for each step in the decontamination process. Pre-cleaning. Manual cleaning. Automated cleaning. Case Solutions. CSR Ink and adhesive remover. SchmutzOff stainless steel, acid based re-conditioner and . Pulsar:. Neutron . star. . with. . offset. . between. . magnetic. . and. . rotation. . axis. .  . emitting. . radio. . waves. in a . cone. (. lighthouse. . effect. ). . Neutron star. 20.11. 1. Neutron stars. T. he . remains of cores of some massive stars that have become supernovae. .. Cores are . a degenerate gas of mostly neutrons.. So much compression at each stage of core contraction that final radius is .