Sentence examples for dense disk from inspiring English sources

Accretion on to black holes and neutron stars is known to produce strong outflows in the form of collimated radio jets and dense disk winds.

Long before any infalling material, whether astronaut or gas cloud, reached the point of no return, it would be accelerated to nearly the speed of light and heated to millions of degrees, sparking X-rays and high-energy particles, as it swirled in a thick dense disk around the cosmic drain.

This petite dessert, neat and precise and surely owing more to France than to Italy, is no mere tart but a true confection, a dense disk of rich yet impossibly light bittersweet chocolate laced with hints of crystal-clear orange, almost as if it were a fleeting thought rather than a flavor.

In the disk model, the gravity of a dense disk of gas around Sgr A* offsets the tidal forces and allows stars to form; in the migration model, the stars formed in a star cluster far away from the black hole and migrated in to form the ring of massive stars.

Afterward, the moon coalesced from impact debris circling Earth in a dense disk.

Gravitational interactions between Neptune and the surrounding dense disk of gas, dust, and small protoplanets would have driven the planet outward to its present position.

Oxygen permeation fluxes through dense disk-shaped Ba0.5Sr0.5Co0.8Fe0.2O3−δ (BSCFO) membranes were investigated as a function of temperature (973 1123 K), pressure (2 10 atm), and membrane thickness (1 2 mm) under an air/helium gradient.

In a denser disk they can transfer energy to electrons--which radiate millions of times more efficiently--but in a rarefied disk, collisions between the protons and electrons would be rare.

(B i v ) Shown are the IL2 plug (B i ; arrow), electron-dense disk at the tip of IL1 and material at the tip of IL2 (B ii, arrow and arrowhead, respectively), rootlet and rootlet-like structures (B iii ; arrowheads); IL1 CeAJ and invaginations into the IL2 PCMC (B iv ; arrow and arrowhead, respectively), and an IL2 CeAJ (B v ; arrow).

Electron-dense disks and precursors of the polar tubule developed in the cytoplasm of the plasmodium prior to budding of early sporoblasts from the plasmodial surface.

Initially, the falling gas forms a thin, dense 'accretion disk' that encircles the compact object and is supported against gravitational collapse by centrifugal force.