Magnetorotational instability in decretion disks of critically rotating stars and the outer structure of Be and Be/X-ray disks

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Table 1

Parameters of Be/X-ray binaries.

Binary	Sp. Type	T _eff	R ¹	D	L _X
		[kK]	[R_⊙]	[R_⊙]	[erg s^-1]


V831 Cas ²	B1V	24	4.5	480	2 × 10³⁵
IGR J16393-4643 ³	BV	24	4.5	18.8	4 × 10³⁵
V615 Cas ⁴	B0Ve	26	4.9	43	5 × 10³⁵
HD 259440 ⁵	B0Vpe	30	5.8	510	1.2 × 10³³
HD 215770 ⁶	O9.7IIIe	28	12.8	260	6.5 × 10³⁶
CPD-632495 ⁷	B2Ve	34	7.0	177	3.5 × 10³⁴
GRO J1008-57 ⁸	B0eV	30	5.8	390	3 × 10³⁷
HD 102567 ⁹	B1Vne	25.5	4.8	240	1.1 × 10³⁵

Reference.

⁽¹⁾

Derived from the effective temperature and spectral type using formulas of Harmanec (1988) and Martins et al. (2005).

⁽²⁾

Reig et al. (1997), Sarty et al. (2009).

⁽³⁾

Combi et al. (2004), Bodaghee et al. (2012), Thompson et al. (2006).

⁽⁴⁾

Zamanov & Martí (2000), Zamanov et al. (2001), Greiner & Rau (2001), Massi (2004).

⁽⁵⁾

Moldón et al. (2011), Casares et al. (2012).

⁽⁶⁾

Caballero et al. (2010), Ikhsanov et al. (2001), Giovannelli et al. (2013).

⁽⁷⁾

Sushch et al. (2012), Sierpowska-Bartosik & Bednarek (2008).

⁽⁸⁾

Coe et al. (2007), Kühnel et al. (2013).

⁽⁹⁾

Stevens et al. (1997), Janot Pacheco et al. (1982).

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