Image Details
Caption: Figure 5.
Radio continuum SEDs for the three regions observed with the GBT in RRLs. The radio continuum data have been convolved to a resolution of ﹩56^{\prime} ﹩. The solid lines show power-law spectra with a spectral index of β = −2.2 normalized to the brightness of the 5 GHz data point. The data for G24.07−0.59 lie behind those for G15.85+0.10.
© 2026. The Author(s). Published by the American Astronomical Society.