Sentence examples for time accretion from inspiring English sources

We have simulated different formation scenarios of Varuna by varying the accretion time, accretion rate, and a fraction of impact kinetic energy converted into heat.

Göpel, C., Manhès, G. & Allègre, C. J. Constraints on the time of accretion and thermal evolution of chondrite parent bodies by precise U Pb dating of phosphates.

More advanced model of Robuchon et al. (2010) further reduces the range of possible time of accretion and indicates that special Burgess rheology is necessary.

This layer would have a fabric anisotropy associated with plate motion at the time of accretion and so could also be electrically anisotropic by shearing.

VPI-2 and VSP-2 seem to have assembled over time by accretion of smaller units, which we call islets.

Time-dependent accretion during the infall phase may account for the low luminosity of Taurus-Auriga protostars; this hypothesis requires more tests.

(2) In addition, we point out that iron lines from time-dependent accretion disks in their "quiescent" states should be narrow even if the cold accretion disk extends to the last stable orbit.

Onset-time of accretion, magnitude and overall behaviour are in excellent agreement, despite the chaotic nature of the turbulent flow.

Also the onset-time of accretion and the saturation values differ significantly between the (N_{theta}=64) run and its high-resolution counterparts.

Due to the high temperature of the gas, the time-averaged accretion rate onto the protostar is of order (1mbox { M}_{odot} mbox { yr}^{-1}), eventually resulting in the formation of a super-massive star.

Up to a mass of about 10 M⊙, the accretion time (t_{mathrm{acc}}=M_/dot{M}_), where (M_) is the mass of the protostar, is smaller than the Kelvin-Helmholtz time (t_{mathrm{KH}}=GM_^{2}/ (R_L_ )), where (L_) is the luminosity of the protostar.