Left panel: continuum emission from L₂ Pup at ν = 338 ± 16 GHz. Right panel: PSF-subtracted continuum emission map. The color scales are a function of the square root of the intensity in mJy beam^-1 km s^-1. The white cross marks the position of the secondary source in the PSF-subtracted ALMA image. The triangular symbols are pointers to the inner rim of the dust disk (6 AU, magenta) and of the secondary source detected in the visible by Kervella et al. (2015; cyan), shifted by −0.1″ in declination. The position of source B from ALMA is marked with a white cross, and the size of the photosphere of the star is shown as a white circle. The 17.7 × 14.5 mas beam is represented in the lower left corner of the images.