Molecules with ALMA at Planet-forming Scales (MAPS): XII. Inferring the C/O and S/H ratios in protoplanetary disks with sulfur molecules

Author(s):
Le Gal, R.; Öberg, K.I.; Teague, R.; Loomis, R.A.; Law, C.J.; Walsh, C.; Bergin, E.A.; Ménard, F.; Wilner, D.J.; Andrews, S.M.; Aikawa, Y.; Booth, A.S.; Cataldi, G.; Bergner, J.B.; Bosman, A.D.; Cleeves, L.I.; Czekala, I.; Furuya, K.; Guzmán, V.V.; Huang, J.; Ilee, J.D.; Nomura, H.; Qi, C.; Schwarz, K.R.; Tsukagoshi, T.; Yamato, Y.; Zhang, K.
Published
2021
Publication type
Article / Letter to editor
Protoplanetary disksPlanet formationInterstellar moleculesRadio astronomyInterferometryAstronomical modelsChemical abundancesInterstellar abundancesAstrochemistry1300, 1241, 849, 1338, 808, 86, 224, 832, 75Astrophysics - astrophysics of galaxiesAstrophysics - Earth and planetary astrophysics
Date issued
2021-11-03
Language
English
Is part of
The Astrophysical Journal Supplement Series (2021), No. 1
hdl
1887/3275432
doi
10.3847/1538-4365/ac2583
URL
https://ui.adsabs.harvard.edu/abs/2021ApJS..257...12L