The GRAVITY young stellar object survey - XIII. Tracing the time-variable asymmetric disk structure in the inner AU of the Herbig star HD 98922

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Table 5

RT results for Model CS.

R_t, M_d,in	5.5 au, 6 × 10^–9 M_⊙				3.5 au, 3 × 10^–9 M_⊙

Flux	SED		Interf.		SED		Interf.
(%)	H	K	H	K	H	K	H	K
Star	30	16	22	23	28	14	22	23
LDC	70	75	78^(*)	77^(*)	41	44	78^(*)	77^(*)
HDC	0	9	–	–	31	42	–	–

Notes. LDC and HDC stand for low-density and high-density component, respectively. The sign^(*) indicates that the relative flux contributions of the disk and halo components are added.

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