A network of filaments detected by Herschel in the Serpens core - A laboratory to test simulations of low-mass star formation

Free Access

Table 4

Standard deviation σ_η (defined in Eq. (3)) of the log-normal distributions overplotted in Figs. 4–7.

	Serpens core	Run I @ t_SC	P_K−S

Entire field	0.27	0.78^a	0.54
Filaments with cores	0.28^b (0.25^c)	0.36	0.03
Filaments without cores	0.24^b (0.25^c)	0.32	0.19
Control field	0.13	0.38	0.36

Notes. The last column shows the probability that the simulated and observational data (the observed filaments refer to numbers 1 to 8) are drawn from the same distribution using the K-S test.

^(a)

σ_η of Run I at t_SC+0.4 Myr is 0.68.

^(b)

Filament numbers 1−8.

^(c)

Filament numbers 2−8 (excluding filament 1).

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.