Other key results concern the discovery on 5 March 1979 of the first pulsating burst, later called Soft Gamma Ray Repeater (SGR), from the supernova remnant N49 in the Large Magellanic Cloud (Mazets et al. 1979b): SGR 0526-66. Konus detected a total of 16 recurrent bursts from this ...
The 7 s X-ray pulsar 1E2259+586 and the supernova remnant (SNR) G109.1-1.0 (CTB109) were observed by BeppoSAX in 1996 November. The pulse period of 6.978914 +/- 0.000006 s implies that 1E2259+586 continues its near constant spin-down trend. The 0.5-10 keV pulse shape is characteriz...
Time zero corresponds to the center of the pulse. Therefore, secondary ionization is an essential physical process in all modelling approaches addressing the behaviour of complex systems under high-intensity irradiation. Even at high X-ray fluence, the volume-integrated ion fragment mass spectra ...
Baylor College of Medicine Human Genome Sequencing Center, Department of Molecular and Human Genetics, One Baylor Plaza, Houston, Texas, 77030, USA Steven Scherer, Donna Muzny, Rui Chen, Andrew Cree, Preethi Gunaratne, Paul Havlak, Anne Hodgson, Michael L. Metzker, Stephen Richards, Graham Scott...
The Einstein Observatory has observed in M31 the same types of strong point X-ray sources that we know in our own galaxy and in the Magellanic Clouds. Their numbers are about 3 times larger (76 vs. 26 sources with Lx > 5 × 1036 ergs/sec) presumably due
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README MIT license Larch: Data Analysis Tools for X-ray Spectroscopy and More Documentation: http://xraypy.github.io/xraylarch Code: http://github.com/xraypy/xraylarch Larch is an open-source library and set of applications for processing and analyzing X-ray absorption and fluorescence spectros...
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The X-ray structure of IPCT/DIPPS revealed a large polar active site cavity that lies near the membrane interface and should be a common feature to other CDP-OH phosphotransferases. This positioning is strategic to allow accommodation and binding of both hydrophilic and lipophilic substrates. The...
Such transient RDKR X-ray source heats periphery of plasma up to hundreds eV temperature keeping it solid (Zone 1). At a greater distance from the center of the plasma (Zones 2 and 3) electron temperature drops to a few eV, and due to efficient pumping by X-ray source hollow ions ...