Formation of close-in super-Earths in evolving protoplanetary disks due to disk winds

Free Access

Table 2

Summary of models.

Model	Disk model	M_tot (M_⊕)	Comments
model1	disk1	80	Standard model
model2	disk2	80	Standard model
model3	disk1	40
model4	disk1	20
model5	disk2	40
model6	disk2	20

model7	disk1	50	r_out = 1 au
model8	disk1	30	r_out = 0.5 au
model9	disk1	17	r_out = 0.3 au
model10	disk1	80	Solid slope = –1
model11	disk1	80	Solid slope = –2

Notes. The first column indicates the model name. The second column indicates the disk model. In disk1 and disk2 models, and 8 × 10⁻⁵ are used, respectively. The third column shows the total mass of initial planetary embryos.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.