Published October 25, 2024
| Version v1
Figure
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The SOFIA Massive (SOMA) Star Formation Q-band Follow-up. I. Carbon-Chain Chemistry of Intermediate-Mass Protostars
Description
These figures show spectra obtained by the Yebes 40m telescope toward eleven intermediate-mass protostars. Black lines indicate the observational spectra and red curves indicate the best-fitting models with the MCMC method. Blue curves show the results of the Gaussian fitting.
Files
fig_carbon3_spec.pdf
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Additional details
Dates
- Accepted
-
2024-10-25