CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy: I. Organic molecules and tracers of star-formation activity

CHEMOUT: CHEMical complexity in star-forming regions of the OUTer Galaxy: I. Organic molecules and tracers of star-formation activity

Context. The outer Galaxy is an environment with metallicity lower than the Solar one. Because of this, the formation and survival of molecules in star-forming regions located in the inner and outer Galaxy is expected to be different. Aims. To gain an understanding on how chemistry changes throughou...

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Bibliographic Details
Main Authors: Beltrán, M.T (Author), Bizzocchi, L. (Author), Caselli, P. (Author), Colzi, L. (Author), Elia, D. (Author), Fontani, F. (Author), Magrini, L. (Author), Rivilla, V.M (Author), Romano, D. (Author), Sánchez-Monge, A. (Author), Testi, L. (Author)
Format: Article
Language:English
Published: EDP Sciences 2022
Subjects:
Astrophysics
Chemical complexity
Galactocentric distances
Galaxies
Giant stars
ISM : clouds
ISM: clouds
ISM: molecules
ISM:molecules
Metallicities
Metals
Molecules
Organic molecules
Organic tracers
Radio lines: ISM
Silicon compounds
Star-forming region
Stars formation
Stars: formation
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