Results 231 to 240 of about 24,589 (267)

Fast sleep spindles as a potential prognostic marker of developmental outcome in infantile epileptic spasms syndrome

open access: yesEpilepsia Open, EarlyView.
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
wiley   +1 more source

Genetic Variants Related to Increased CKD Progression-A Systematic Review. [PDF]

open access: yesBiology (Basel)
Mira FS   +4 more
europepmc   +1 more source

Gesture Imitation Performance and Visual Exploration in Young Children with Autism Spectrum Disorder. [PDF]

open access: yesJ Autism Dev Disord
Latrèche K   +6 more
europepmc   +1 more source

Cyclic Amide-Linked Oxazolidinone Triazoles as Inhibitors of the T-Box Riboswitch. [PDF]

open access: yesMolecules
Parsons E   +6 more
europepmc   +1 more source

The accretion geometry of intermediate polars (DQ her stars)

Advances in Space Research, 1988
The 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
openaire   +1 more source

The DQ Herculis stars

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
openaire   +1 more source

On the Optical Pulsations in DQ Her Stars

1995
DQ 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
openaire   +1 more source

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