The interplay between disk wind and magnetospheric accretion mechanisms in the innermost environment of RU Lup

Home

All issues

Volume 689 (September 2024)

A&A, 689 (2024) A124

Full HTML

Open Access

Table A.1

Magnetospheric accretion model response properties.

	P_r	ΔP	ΔFlux	ΔSize	ΔPC	Mean Δ	ξ _Flux	ξ_Size	ξ_PC	ξ_tot
		[%]	[%]	[%]	[%]	[%]	[%]	[%]	[%]	[%]
T_mag	8600 K	16	22	27	73	41	134	167	448	250
R_*	2.5 R_⊙	24	5	21	27	17	22	86	111	73
R_mi	7 R_*	43	10	29	39	26	23	69	90	61
P_*	7 days	45	3	6	38	16	7	14	84	35
${\dot{M}}_{a c c}$ $\[\dot{M}_{a c c}\]$	23 10⁻⁸ M_⊙yr⁻¹	22	8	4	11	8	35	16	52	35
δR_m	2 R_*	50	12	4	26	14	24	8	51	28
M_*	0.8 M_⊙	38	7	4	12	8	20	10	32	21
T_*	4050 K	2	0	0	0	0	2	0	4	2

Average		30	8	12	28	16	33	46	109	63

Notes. All quantities marked with Δ are mean parameter variations of the magnetospheric accretion model, given in relation to the reference parameter P_r. ξ denotes the resulting responses of the computed synthetic observables (line-to-continuum flux ratio, characteristic emission region size, and emission region offset), as computed according to Eq. A.2.

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.