A far-infrared survey of bow shocks and detached shells around AGB stars and red supergiants

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201117910e]

Table 8

Two-sample Kolmogorov-Smirnov test applied to different stellar, circumstellar, and interstellar parameters possibly relevant to “detection” and “non-detection” samples (distance d ≤ 500 pc).

	Kolmogorov probability p ^a

	(I, II, IV)	(I, II, IV)	(III)	(I–IV)
	vs. (III)	vs. (X)	vs. (X)	vs. (X)
	n = (34,8)	n = (34,16)	n = (8,16)	n = (42,16)

critical value (α = 0.01)	0.70	0.56	0.76

d (pc)	0.25	0.18	0.98	0.28
z (pc) / n_H (cm^-3)	0.99	0.03	0.19	0.02
v_⋆ (km s^-1)	0.43	0.02	0.09	0.02
inclination i (°)	0.01	0.52	0.19	0.68
Ṁ(M_⊙ yr^-1)	0.55	0.48	0.59	0.57
v_w (km s^-1)	0 78	0.74	0.84	0.78
R₀ predicted (pc)	0.40	0.07	0.84	0.09
R₀ predicted (arcmin)	0.94	0.02	0.19	0.02

Notes.

^(a)

The second to fifth columns give the K-S results between different sub-sets of classes (see Table 4 for the classification). The number of data-points in each (sub)set are given in the fourth row.

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