Nonradial and nonpolytropic astrophysical outflows - X. Relativistic MHD rotating spine jets in Kerr metric

Free Access

Table 2

Output parameters for the four solutions in the Kerr metric.

	ϵ	m₁	Π_⋆,lim	r₀∕r_s
K1	− 1.76	− 0.062	0.826	5.72

K2	− 0.04	− 0.234	0.216	1.57

K3	0.55	− 0.326	0.189	2.55

K4	− 5.84	− 0.004	0.255	1.39

Notes. Those parameters result from the integration of the equations.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.