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

Le Gal, R.; Öberg, K.I.; Teague, R.; Loomis, R.A.; Law, C.J.; Walsh, C.; ... ; Zhang, K. (2021)

Article / Letter to editor

• Protoplanetary disks
• Planet formation
• Interstellar molecules
• Radio astronomy
• Interferometry
• Astronomical models
• Chemical abundances
• Interstellar abundances
• Astrochemistry
• 1300, 1241, 849, 1338, 808, 86, 224, 832, 75
• Astrophysics - astrophysics of galaxies
• Astrophysics - Earth and planetary astrophysics

• All authors: 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.
• Date: 2021-11-03
• Journal: The Astrophysical Journal Supplement Series
• Volume: 257
• Issue: 1
• DOI: doi:10.3847/1538-4365/ac2583
• Link: https://ui.adsabs.harvard.edu/abs/2021ApJS..257...12L