Image Details
Caption: Figure 6.
Emission lines of N-bearing molecules CH3CN, C2H5CN, C2H3CN, NH2CN, NH2CHO, and HC3N (ν7 = 2). The green lines indicate the observed molecular spectra of NIRS3, and the blue lines represent the LTE model spectra of detected N-bearing species. Red spectra are the LTE model spectra of all species, including detected N-bearing molecules. The systemic velocity of the spectra is 5.0 km s−1.
© 2026. The Author(s). Published by the American Astronomical Society.