ALMA observation of an evolving magnetized corona in the radio-quiet changing-state active galactic nucleus NGC 1566

Open Access

Fig. 1.

ALMA image of NGC 1566 in band 6 at 230 GHz, observed on 2022-06-14. The synthesized beam size (gray ellipse at the lower corner) is $0 \binom{″}{\cdot} 44 \times 0 \binom{″}{\cdot} 29$ $0{{\prime\prime \atop \cdot }} 44 \times 0{{\prime\prime \atop \cdot }} 29$ (38×25 pc). The contours of the emission are drawn at (3, 10, 20)σ, where σ = 0.1 mJy beam⁻¹. For NGC 1566, 1 arcsec angular width corresponds to 87 pc in physical scale.

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.