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astro-ph.GA2026
Discovery of thermal radio recombination line emission toward the high-mass protostar IRAS181622048
R. Fedriani, J. F. Gomez, Y. Cheng +7
The physical conditions within the innermost few tens of au of high-mass protostars () remain largely unexplored. At these scales, ionised emission may trace photoio…
astro-ph.GA2025
Diverse stages of star formation in the IRAS 18162-2048 region. Emergence of UV Feedback
R. Fedriani, G. Anglada, A. Caratti o Garatti +15
Methods: We obtained adaptive optics-assisted integral field spectroscopy in the near-infrared (IR) band () with VLT/SINFONI, complemented by VLA X and C…