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Fragmentation during the accretion phase may further reduce the mass of the central protostar.
Consequently, the subaerial Yellow River delta transitioned to a slight accretion phase.
Numerical simulations of gravitational compaction during the sediment accretion phase as well as along geological period of pore pressure dissipation are performed in the context of oedometric setting.
I then review the influence of fragmentation on the accretion phase, the evolution of the nascent protostellar system, and the effects of protostellar radiation on the initial mass function (IMF) of the first stars (Section 3).
Due to the Courant constraint, it is not possible to model the accretion phase accurately for more than a few free-fall times, or ({simeq}10mbox { yr}) (Ripamonti et al. 2002; Greif et al. 2012).
PPF of GCNP has passed through an accretion phase of forest development with increases in density and, depending on PPF subtype and variable being examined, is at or past the point of inflection to recession of density and basal area.
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During the gas-accretion phase of giant planet formation the star planet contrast may be even better in H alpha than it is in infrared – an H alpha survey is currently underway.
Two high-energy growth phases (U3 and U4) that combine progradation and accretion form the present-day external bank shape.
Various authors show that the increase of dust mass in the Milky Way ISM is mainly governed by grain growth through the accretion of gas phase metals onto the grains (elements comprised of dust grains are referred to as "metals") (Dwek, 1998; Inoue, 2003; Zhukovska et al., 2008; Draine, 2009; Inoue, 2011; Asano et al., 2013).
Various authors show that the increase of the total dust mass in the Milky Way ISM is mainly governed by grain growth through the accretion of gas phase metals onto the grains (we call elements composing dust grains "metals") (e.g., Dwek, 1998; Zhukovska et al., 2008; Inoue, 2011; Asano et al., 2013a).
They used the method to simulate the evolution of the grain mantle by one-by-one accretion of gas phase species and calculating their fate (reaction, desorption, trapping) before a new species would land on the surface.
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Justyna Jupowicz-Kozak
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