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Modelling the abundance structure of isocyanic acid (HNCO) toward the low-mass solar type protostar IRAS 16293-2422
Antonio Hernández-Gómez, Emna Sahnoun, Emmanuel Caux +5
Isocyanic acid (HNCO), the most stable of the simplest molecules containing the four main elements essential for organic chemistry, has been observed in several astrophysical envir…
3D modelling of HCO and its isotopologues in the low-mass proto-star IRAS162932422
D. Quénard, S. Bottinelli, E. Caux +1
Ions and electrons play an important role in various stages of the star formation process. By following the magnetic field of their environment and interacting with neutral species…
Seeds of Life in Space (SOLIS). III. Zooming into the methanol peak of the pre-stellar core L1544
Anna Punanova, Paola Caselli, Siyi Feng +41
Towards the pre-stellar core L1544, the methanol (CHOH) emission forms an asymmetric ring around the core centre, where CHOH is mostly in solid form, with a clear peak 4000…