Magnetism in clean energy and environment

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DIFFERENCES BETWEEN RADIO-LOUD AND RADIO-QUIET γ-RAY PULSARS AS REVEALED BY <i>FERMI</i>

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CHANDRA DETECTION OF A NEW DIFFUSE X-RAY COMPONENT FROM THE GLOBULAR CLUSTER 47 TUCANAE

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Gamma-Ray Emission of the Kes 73/1E 1841-045 Region Observed with the Fermi Large Area Telescope

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HIGH-ENERGY EMISSIONS FROM THE GAMMA-RAY BINARY LS 5039

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X-ray Studies of the Black Widow Pulsar PSR B1957+20

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XMM-Newton observation of PSRB2224+65 and its jet

We have investigated the pulsar PSRB2224+65 and its X-ray jet with XMM-Newton. Apart from the long X-ray jet which is almost perpendicular to the direction of proper motion, a putative extended feature at the pulsar position, which is oriented in the opposite direction to the proper motion, is also suggested by this deep X-ray imaging. Non-detection of any coherent X-ray pulsation disfavors the magnetospheric origin of the X-rays observed from the position of PSRB2224+65 and hence suggests that the interpretation of pulsar wind nebula is more viable. We have also probed the origin of PSRB2224+65 and identified a runaway star, which possibly originated from the Cygnus OB9 association, as a candidate for the former binary companion of the neutron star's progenitor. © 2012. The American Astronomical Society. All rights reserved.postprin

Fermi-lat Detection Of Pulsed Gamma-rays Above 50 Gev From The Vela Pulsar

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Search for pulsed γ-ray emission from globular cluster M28

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Exploring the X-ray and γ-ray properties of the redback millisecond pulsar PSR J1723-2837

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