Image Details
Caption: Figure 3.
Top: comparison between formaldehyde column density in the two 100 au radial bins, with the dashed line indicating the identity. Bottom: excitation temperature of H2CO between the inner 100 au and the successive 100–200 au radial bin. No significant difference between the two temperatures can be stated given the uncertainties due to the lower SNR of the emission in the outer 100 au.
© 2026. The Author(s). Published by the American Astronomical Society.