Investigating the rotational evolution of very low-mass stars and brown dwarfs in young clusters using Monte Carlo simulations

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Table 4

Observational data for VLM stars and BDs used for period comparison.

Region	Age	Numbers		Mass range	Ref.
	(Myr)	VLM	BD	(M_⊙)

ONC	1–3	445	79	0.02–1.5^a	1
ONC	1–3	135	–	0.1–3.0^a	2
σ Ori	3–6	10	9	0.02–0.7^a	3
σ Ori	3 –6	37	10	0.02–0.5^a	4
NGC 2362	5	70	–	0.1–1.2^a	5
Upper Sco	5–11	–	16	0.02–0.09	7

Notes.

^(a)

We restrict the mass range up to 0.4 M_⊙.

Reference. (1) Rodríguez – Ledesma et al. (2010, RL10); (2) Davies et al. (2014, D14); (3) Scholz & Eislöffel (2004, S04); (4) Cody & Hillenbrand (2010, C10); (5) Irwin et al. (2008, I08); (7) Scholz et al. (2015, S15).

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