Unlocking the sulphur chemistry in intermediate-mass protostars of Cygnus X. Connecting the cold and warm chemistry

Autor: M. el Akel, L. E. Kristensen, R. Le Gal, S. J. van der Walt, R. L. Pitts, F. Dulieu

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 659 (A100), ⟨10.1051/0004-6361/202141810⟩
el Akel, M, Kristensen, L E, Le Gal, R, van der Walt, S J, Pitts, R L & Dulieu, F 2022, ' Unlocking the sulphur chemistry in intermediate-mass protostars of Cygnus X Connecting the cold and warm chemistry ', Astronomy & Astrophysics, vol. 659, A100 . https://doi.org/10.1051/0004-6361/202141810

Context. The chemistry of sulphur-bearing species in the interstellar medium remains poorly understood, but might play a key role in the chemical evolution of star-forming regions. Aims. Coupling laboratory experiments to observations of sulphur-bear

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https://hal-insu.archives-ouvertes.fr/insu-03672048