Image Details
Caption: Figure 2.
Total flux density and angular size as a function of frequency for the continuum emission of MWC 349A. The solid lines are the linear least-squares fits to the data from this study and data from previous studies; the dashed lines are the linear least-squares fits found by Tafoya et al. (2004).
© 2023. The Author(s). Published by the American Astronomical Society.