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Abstract Objective The presence or absence of sleep spindles in patients with infantile epileptic spasms syndrome (IESS) has been proposed as a potential predictor of cognitive outcome; however, the validity of this predictor remains uncertain.
Kento Ohta +6 more
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Genetic Variants Related to Increased CKD Progression-A Systematic Review. [PDF]
Mira FS +4 more
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Global conformations of <i>Pichia pastoris</i> complex I are distinguished by the binding of a unique interdomain bridging subunit. [PDF]
Lee CS +4 more
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Revealing Cycling-Induced Evolution of Intact Sodium Metal Battery Interfaces Using Cryo-Focused Ion Beam Cross-Sectioning and Electron Microscopy. [PDF]
Matthews KC +3 more
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Gesture Imitation Performance and Visual Exploration in Young Children with Autism Spectrum Disorder. [PDF]
Latrèche K +6 more
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Cyclic Amide-Linked Oxazolidinone Triazoles as Inhibitors of the T-Box Riboswitch. [PDF]
Parsons E +6 more
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The accretion geometry of intermediate polars (DQ her stars)
Advances in Space Research, 1988The Cataclysmic Variables (CV) are interacting binary systems in which a white dwarfstar accretes matter from a red dwarf companion that is filling its Roche limiting surface (for reviews see /1/ /2/ /3/). It has become apparent in recent years that the white dwarfstar in some CV has a magnetic field which is strong enough to influence the flow of ...
K.O. Mason, S.R. Rosen, C. Hellier
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Publications of the Astronomical Society of the Pacific, 1994
We review the properties of the DQ Herculis stars: cataclysmic variables containing an accreting, magnetic, rapidly rotating white dwarf. These stars are characterized by strong X-ray emission, high-excitation spectra, and very stable optical and X-ray pulsations in their light curves. There is considerable resemblance to their more famous cousins, the
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We review the properties of the DQ Herculis stars: cataclysmic variables containing an accreting, magnetic, rapidly rotating white dwarf. These stars are characterized by strong X-ray emission, high-excitation spectra, and very stable optical and X-ray pulsations in their light curves. There is considerable resemblance to their more famous cousins, the
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On the Optical Pulsations in DQ Her Stars
1995DQ Her stars are cataclysmic binary systems in which matter from a late-type near-main sequence star is accreted onto an asynchronously spinning magnetized white dwarf. X-rays generated at shocks at the magnetic poles of the white dwarf sweep the system with a “lighthouse” beam, producing optical signals modulated at the spin period of the white dwarf ...
Phillip J. Martell, William F. Welsh
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