EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 706 (February 2026) A&A, 706 (2026) A57 Full HTML
Open Access

Table 1

Parameter ranges for the magnetospheric accretion models (Thanathibodee et al. 2019a) and best-fit results.

Rin Width Ṁ Tcol i Mp Rp Lacc
(Rp) (Rp) (M⊙/yr) (K) (∘) (MJup) (RJup) (L⊙)
Range 1.5–6.0 0.5–2.5 9.5 × 10−(13–10) 6000–10 000 15–75 11–15 1.4–1.6
Hα Wings ±50 km/s 2.0 2.0 6.02 × 10−12 9250 60 15 1.4 1.88 × 10−5
Hα Wings ±250 km/s 1.5 1.0 1.51 × 10−12 10 000 75 15 1.4 4.72 × 10−6
Hα Core ±50 km/s 3.0 0.5 1.51 × 10−12 8750 30 15 1.6 4.13 × 10−6
Hα Core ± 250 km/s 1.5 0.5 3.80 × 10−10 6000 75 11 1.6 7.62 × 10−4
Hβ Wings ±50 km/s 1.5 2.5 1.51 × 10−10 8000 75 13 1.5 3.82 × 10−4
Hβ Wings ±250 km/s 2.0 2.5 9.55 × 10−10 10 000 75 15 1.6 2.61 × 10−3
Hβ Core ±50 km/s 2.0 0.5 9.55 × 10−13 10 000 30 13 1.4 2.59 × 10−3
Hβ Core ± 250 km/s 2.0 0.5 9.55 × 10−10 6250 75 11 1.5 2.04 × 10−3

Notes. Results are shown for the wing and core components, in the (−50, +50) km/s and (−250, +250) km/s cases, for both Hα and Hβ. The accretion luminosity Lacc was computed as Lacc=GṀMp/Rp. For the full χr2$\chi^2_r$ space, see Figs. F.1 and F.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.