A rich hydrocarbon chemistry and high C to O ratio in the inner disk around a very low-mass star

Author(s):
Tabone, B.; Bettoni, G.; Dishoeck, E.F. van (0000-0001-7591-1907); Arabhavi, A.M.; Grant, S.; Gasman, D.; Henning, T.; Kamp, I.; Güdel, M.; Lagage, P.O.; Ray, T.; Vandenbussche, B.; Abergel, A.; Absil, O.; Argyriou, I.; Barrado, D.; Boccaletti, A.; Bouwman, J.; Caratti o Garatti, A.; Geers, V.; Glauser, A.M.; Justannont, K.; Lahuis, F.; Mueller, M.; Nehmé, C.; Olofsson, G.; Pantin, E.; Scheithauer, S.; Waelkens, C.; Waters, L.B.F.M.; Black, J.H.; Christiaens, V.; Guadarrama, R.; Morales-Calderón, M.; Jang, H.; Kanwar, J.; Pawellek, N.; Perotti, G.; Perrin, A.; Rodgers-Lee, D.; Samland, M.; Schreiber, J.; Schwarz, K.; Colina, L.; Östlin, G.; Wright, G.
Published
2023
Publication type
Article / Letter to editor
Astrophysics - Earth and Planetary AstrophysicsAstrophysics - Solar and Stellar Astrophysics
Date issued
2023
Language
English
Is part of
Nature Astronomy (2023), Vol. 7, p. 805-814
hdl
1887/3715489
doi
10.1038/s41550-023-01965-3
URL
https://ui.adsabs.harvard.edu/abs/2023NatAs...7..805T