A dusty magnetospheric stream explaining the light curves of the dipper objects: Finding a new inclination threshold to produce dippers

Open Access

Fig. 7

Grain opacity multiplied by their abundance along the accretion stream is shown for the stellar Model 2 with M_★ = 0.178 M_⊙ and Model 14 with M_★ = 0.832 M_⊙. The color scale represent the opacity in units of cm² g⁻¹.

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