(i) Cold, COM-poor sources
(ii) Warm, medium-COM-abundance sources
(iii) Hot, COM-rich sources
These groups hint at different evolutionary stages in massive star formation.
(i) Cold, COM-poor sources
(ii) Warm, medium-COM-abundance sources
(iii) Hot, COM-rich sources
These groups hint at different evolutionary stages in massive star formation.
We're excited to share our latest work at UdeA, recently published in Astronomy & Astrophysics. We show how machine learning can cut down the manual workload in rotational diagram analysis, directly decoding mm-wave spectra! 🧵 #Astronomy
We're excited to share our latest work at UdeA, recently published in Astronomy & Astrophysics. We show how machine learning can cut down the manual workload in rotational diagram analysis, directly decoding mm-wave spectra! 🧵 #Astronomy