Interaction between the ejecta, the accretion disk, and the secondary star in the recurrent nova system U Sco

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Table 1.

U Sco models computed.

Model	M_ejecta	$V_{ejecta}^{\max}$ $V_{\mathrm{ejecta}}^{\mathrm{max}}$	ρ_ejecta	M_disk	Shape disk
	(M_⊙)	(km s⁻¹)		(M_⊙)
A	2.1 × 10⁻⁶	10 000	`SHIVA`	10⁻⁶	Flared
B	1.1 × 10⁻⁶	10 000	`SHIVA`	10⁻⁶	Flared
C	2.1 × 10⁻⁶	5000	`SHIVA`	10⁻⁶	Flared
D	2.1 × 10⁻⁶	2000	`SHIVA`	10⁻⁶	Flared
E	2.1 × 10⁻⁶	10 000	`SHIVA`	4.4 × 10⁻⁶	Flared
F	2.1 × 10⁻⁶	10 000	Const.	10⁻⁶	V-Shaped
G	2.1 × 10⁻⁶	10 000	Const.	10⁻⁶	Flared
H	2.1 × 10⁻⁶	10 000	`SHIVA`	10⁻⁶	V-Shaped

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