Dwarf nova outbursts in intermediate polars | Astronomy & Astrophysics (A&A)

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Table 2

Model parameters and results.

Nr	P _orb	q	μ ₃₃	α _c	α _h	Ṁ _tr	Ṁ _max ^a	log Ṁ_min ^b	τ _rec ^c	Duration^d	Ω_K(r_mag)	νΣ ^e
	(h)					(10¹⁶ g / s)	(10¹⁶ g / s)	(g/s)	(day)	(day)	(mHz)

1	6	0.6	0	0.02	0.1	10	59	12.25	62.2	9.70	–	0
2	6	0.6	0.01	0.02	0.1	10	71	14.76	87.8	12.9	43.0	0
3	6	0.6	0.1	0.02	0.1	10	100/87	15.56	197/95	15.8/4.8	13.2	0
4	6	0.6	0.1	0.04	0.2	10	88	15,61	54.1	6.2	13.8	0
5	6	0.6	0.1	0.01	0.1	10	182/153	15,40	346.8/173.4	13.7/4.7	11.2	0
6	6	0.6	0.1	0.02	0.2	10	184/157	15.45	196/98	8.0/2.5	11.8	0
6	6	0.6	0.1	0.02	0.1	10	59.8	15.76	83.2	14.2	16.0	Ṁ/ 3π
6	6	0.6	0.1	0.02	0.1	2	66,9/29,6	15.42	678/333	15.8/3.7	11.5	Ṁ/ 3π
7	6	0.6	0	0.02	0.1	2	86/1.6	12.25	1217/56.5	15.2/1.9	–	0
8	6	0.6	0.01	0.02	0.1	2	84/37	14,76	1269/254	15.5/6.4	43.0	0
9	1.5	0.2	0	0.02	0.1	5	5.2	12,25	60.4	5.8	–	0
10	1.5	0.2	0.01	0.02	0.1	5	12	14,72	377.5	10.1	41.3	0
11	1.5	0.2	0.01	0.02	0.1	5	4.7	14.76	92.2	9.1	43.0	Ṁ/ 3π

Notes. When there is a sequence of large and smaller outbursts, the first number refers to the properties of the largest outbursts, the second to the smallest ones.

^(a)

Peak accretion rate during outbursts.

^(b)

Minimum mass accretion rate during quiescence.

^(c)

When there is a sequence of large and smaller outbursts, the first number is the time interval between large outbursts and the second the minimum time interval between consecutive outbursts.

^(d)

Outburst duration.

^(e)

Boundary condition at inner disc edge.

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