Sentence examples for embryo embryo from inspiring English sources

Fifty-four datasets, including 30 RNA-seq experiments performed in 13 different tissues (leaf, immature ear, immature tassel, seed, endosperm, embryo, embryo sac, anther, ovule, pollen, silk, root and shoot apical tissues), were applied to construct a co-expression network between lincRNAs acting as miRNA targets and mRNA genes [ 58– 63].

For FRAP in the embryo, embryos were collected overnight, dechorionated and mounted on glass coverslips (20×50 mm) coated with heptane glue.

In summary, our data collection covers the major stages of Drosophila development: pre-embryo, embryo, larva, and pharate adult (Table 1).

In models with smaller embryo masses (model 4 1 0.25 7, Fig. 5a), there are more embryos and therefore more embryo-embryo collisions.

Only embryo-embryo collisions that form the final Earth-like planet are shown.

When there are fewer embryo-embryo collisions, there are more planetesimal impacts in global magma oceans.

Fig. 3 Time until the next impact versus magma ocean crystallisation time for Earth-building giant impacts (embryo-embryo collisions).

Planetesimal impact in a magma ocean that survives from a previous embryo-embryo collision: Equilibration will take place at the base of the magma ocean.

The equilibration pressures for almost all collisions are then dominated by the initial depths of the melt pools that are created by embryo-embryo collisions (i.e. giant impacts).

However, most embryo-embryo collisions that result in shallower melt pools still melt the deep mantle with equilibration taking place at pressures close to the CMB pressure.

Embryo-embryo collisions (large symbols) are visible as maxima, whereas the planetesimal impacts in a residual magma ocean result in a decreasing equilibration pressure with increasing time.