'Bursts' presentation slideshows

Astronomy 350 Cosmology

Astronomy 350 Cosmology. Professor Lynn Cominsky Department of Physics and Astronomy Offices: Darwin 329A and NASA EPO (707) 664-2655 Best way to reach me: lynnc@charmian.sonoma.edu. Group 6. Justin Beck Tiffany Henning Pamela Riek Ryan Silva. Great job group 6!.

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Astronomy 305/Frontiers in Astronomy

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Magnetars are magnetically powered, rotating neutron stars

Magnetars are magnetically powered, rotating neutron stars. RADIO PULSARS 2000 discovered to date Radiate covering most of the electromagnetic spectrum Rotate with periods that span five decades (ms to a few hours). Are powered by their own rotational energy,

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Lecture 4. Magnetars: SGRs and AXPs

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COSMIC GAMMA-RAY BURSTS The Current Status

COSMIC GAMMA-RAY BURSTS The Current Status. Kevin Hurley UC Berkeley Space Sciences Laboratory. SOME ABSOLUTELY INCONTROVERTIBLE GRB PROPERTIES THAT NO REASONABLE PERSON COULD POSSIBLY DISAGREE WITH.

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Superbursts: Nuclear Fury on Neutron Stars

Superbursts: Nuclear Fury on Neutron Stars. Sources of Thermonuclear Bursts: LMXBs Containing Neutron Stars. X-ray binaries near the Galactic center as seen with RXTE/PCA. Accreting neutron stars in low mass X-ray binaries. Roughly 70 burst sources known.

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Abbas Askar abbas.askar@gmail University of Belgrade

X-ray Bursts: Thermonuclear Burning on Neutron Stars. Abbas Askar abbas.askar@gmail.com University of Belgrade. About Astromundus !. 2-year Erasmus Mundus Masters Course in Astronomy and Astrophysics that started in Fall 2010. 3 semesters of courses+1 semester for thesis

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Cape Elizabeth Schools Project Build

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Hard X-ray Tails in Magnetars

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Monitoring the high energy transient sky with the 9-spacecraft interplanetary network

Monitoring the high energy transient sky with the 9-spacecraft interplanetary network. AGILE Fermi INTEGRAL RHESSI. MESSENGER Swift Suzaku Odyssey. Wind.

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Progress on Burst Simulation

Progress on Burst Simulation. Alan Weinstein, Caltech, 3/20/02. t-f character of burst waveforms Burst waveforms Calibration E7 data LDAS jobs Results from TFClusters More work to be done. t-f character of burst waveforms (relevant for astrophysics-based analysis).

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Constructing an Anonymous Dataset From the Personal Digital Photo Libraries of Mac App Store Users

Slides Available : http://bit.ly/ 1aIC3S6. Constructing an Anonymous Dataset From the Personal Digital Photo Libraries of Mac App Store Users. JCDL 2013 Jesse P. Gozali, Min-Yen Kan, Hari Sundaram National University of Singapore, Arizona State University. 1.

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Science Requirements for Estremo

Science Requirements for Estremo. X-RAY BURST PHYSICS. Detection of redshifted lines in X-ray bursts may provide information on NS mass and radius discrete spectral features in a superburst from 4U1820-30 (6.4 keV line + abs edge) observed by RXTE

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The 2006-12-13 event included major flare, fast CME, strong shock, big SEP event and GLE70.

Dedicated to the memory of T. Kosugi. Eruptions, shock waves, and major flare in the 2006-12-13 event V. Grechnev, V.Kiselev, A.Uralov, N.Meshalkina. The 2006-12-13 event included major flare, fast CME, strong shock, big SEP event and GLE70. We endeavor:

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(1) Institute of Radio Astronomy, Kharkov, Ukraine (2) Space Research Institute, Graz, Austria

Decameter Type IV bursts: Properties of Fiber Bursts. V.N. Melnik (1), A.A. Konovalenko (1), H.O. Rucker (2), E.P. Abranin (1), V.V. Dorovskyy (1), F.F.Stanislavskyy (1). (1) Institute of Radio Astronomy, Kharkov, Ukraine (2) Space Research Institute, Graz, Austria. UTR-2 radio telescope.

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Gamma Ray Bursts

1. Gamma Ray Bursts. Ashley S. Pagnotta Texas A&M University November 25, 2003. All sources cited at end. What is a Gamma Ray Burst?.

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Gamma-Ray Bursts

Gamma-Ray Bursts. Discovered by DoD satellites searching for signs of atmospheric nuclear testing irregular bursts of gamma-ray radiation lasting from milliseconds to seconds originally thought to be more energetic versions of X-ray bursts

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(1) I nstitute of Radio Astronomy of NANU, Kharkov, Ukraine

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R E F E R E N C E S

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TYPE IV BURSTS AT FREQUENCIES 10-30 MHz

TYPE IV BURSTS AT FREQUENCIES 10-30 MHz V.N. Melnik (1), H.O. Rucker (2), A.A. Konovalenko (1), E.P. Abranin (1), V.V. Dorovskyy(1), A. A. Stanislavskyy (1), A. Lecacheux (3) Institute of Radio Astronomy, Ukrainian Academy of Sciences, Kharkov, Ukraine;

103 views • 1 slides