MINDS. The detection of ^13CO_2 with JWST-MIRI indicates abundant CO_2 in a protoplanetary disk

Author(s):
Grant, S.L.; Dishoeck, E.F. van (0000-0001-7591-1907); Tabone, B.; Gasman, D.; Henning, T.; Kamp, I.; Güdel, M.; Lagage, P.O.; Bettoni, G.; Perotti, G.; Christiaens, V.; Samland, M.; Arabhavi, A.M.; Argyriou, I.; Abergel, A.; Absil, O.; Barrado, D.; Boccaletti, A.; Bouwman, J.; o Garatti, A.C.; Geers, V.; Glauser, A.M.; Guadarrama, R.; Jang, H.; Kanwar, J.; Lahuis, F.; Morales-Calderón, M.; Mueller, M.; Nehmé, C.; Olofsson, G.; Pantin, E.; Pawellek, N.; Ray, T.P.; Rodgers-Lee, D.; Scheithauer, S.; Schreiber, J.; Schwarz, K.; Temmink, M. (0000-0002-7935-7445); Vandenbussche, B.; Vlasblom, M.; Waters, L.B.F.M.; Wright, G.; Colina, L.; Greve, T.R.; Justannont, K.; Östlin, G.
Published
2023
Publication type
Article / Letter to editor
Protoplanetary disksPlanet formation13001241Astrophysics - Solar and Stellar AstrophysicsAstrophysics - Earth and Planetary Astrophysics
Date issued
2023
Language
English
Is part of
Astrophysical Journal Letters (2023), No. 1, L6
hdl
1887/3716116
doi
10.3847/2041-8213/acc44b
URL
https://ui.adsabs.harvard.edu/abs/2023ApJ...947L...6G