Table 4.
Best fit parameters and central 95% credible interval for the modelling of the spectrum and differential visibility amplitude of NGC 3783.
Parameters | Best fit values |
---|---|
FWHMcont (mas) |
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FWHM[Ca VIII] (mas) |
![]() |
FWHMBrγ, n (mas) |
![]() |
FWHMline,[Ca VIII] (km s−1) |
![]() |
FWHMline, Brγ, b (km s−1) |
![]() |
FWHMline, Brγ, n (km s−1) |
![]() |
ABrγ, n |
![]() |
vBrγ, n (km s−1) |
![]() |
ABrγ, b |
![]() |
vBrγ, b (km s−1) |
![]() |
A[Ca VIII] |
![]() |
v[Ca VIII] (km s−1) |
![]() |
V0, Brγ |
![]() |
V0,[Ca VIII] |
![]() |
Notes. ABrγ, n, ABrγ, b, A[Ca VIII] are the amplitudes of the narrow Brγ, broad Brγ, and [Ca VIII] lines and vBrγ, n, vBrγ, b, v[Ca VIII] are their central velocities relative to the redshift of NGC 3783.
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