ABSTRACT We explore the pulsationally driven orbital mass ejection mechanism for Be star disc formation using isothermal, 3D magnetohydrodynamic (MHD) and hydrodynamic simulations. Non-radial pulsations are added to a rotating at 95 per cent of critical as an inner boundary condition that feeds gas into domain. In MHD, initial magnetic field within is weak. The hydrodynamics simulation has limi...

conclusion adc, fa, and t2* values may quantitatively reflect the microstructural characteristics of np, therefore they could be used to detect the minimal changes of early ldd. results the adc, fa, and t2* values were different (p < 0.05) among different rois within the same disc or among corresponding rois in different level discs. while the average values of adc increased regularly with the ...

I review the observational evidence for spiral structure in the accretion discs of cataclysmic variables (CVs). Doppler tomography is ideally suited to resolve and map such co-rotating patterns and allows a straightforward comparison with theory. The dwarf nova IP Pegasi presents the best studied case, carrying two spiral arms in a wide range of emission lines throughout its outbursts. Both arm...

Imaginal discs of insccts have long been known to be embryonic Anlagen (1). Indeed, in Drosophila, the external structures in the head and thoracic regions, as well as some in the abdominal region, develop from imaginal discs (2). Discs develop normally when transplanted into larvae, and Schneider (3) has recently shown that eye discs develop normally and become pigmented in a defined medium. T...

In this paper, I review our understanding of how jet feedback works in star-forming galaxies. There are some interesting differences to radiative from Active Galactic Nuclei (AGN). Jets act on galaxy haloes as well dense gas, for example regularly rotating discs, where they can suppress star formation (particularly the centre, negative feedback), but also enhance it (positive feedback). Jet may...

BACKGROUND Herniated discs may exhibit calcification, and calcified discs may complicate surgical treatment. However, the osteogenic potential and expression of osteogenic markers in degenerative discs of different degenerative grades are still unclear. Our purposes are to study the differences in calcification rate and osteogenic potential of herniated discs according to different degenerative...

One-third of the people with an age over twenty have some signs of degenerated discs. However, in most of the patients the mere presence of degenerative discs is not a problem leading to pain, neurological compression, or other symptoms. This paper presents an interval type-2 fuzzy hybrid rule-based system to diagnose the abnormal degenerated discs where pain variables are represented by interv...

ABSTRACT We use H i absorption along the lines-of-sight to Q0107 quasar triplet in order model potential disc and outflow structures circumgalactic medium of intervening galaxies at z ? 1, as well intergalactic on scales up a few virial radii. consider sample twelve isolated field with position angles inclinations measured from HST imaging redshifts our spectroscopic surveys, alongside 27 detec...

background: intervertebral disc herniation has two common types, extrusion and protrusion, which may affect the adjacent vertebrae.in addition, it is associated with significant signal changes in t1 mri (short tr/te) and t2 mri (long tr/te).   methods: the present study is a cross-sectional analytic one, in which sampling was performed retrospectively. cases were randomly selected from the pati...