Showing 1–20 of 48 results
/ Date/ Name
Jul 6, 2023Large Myr-old Disks are Not Severely Depleted of gas-phase CO or carbonFeb 1, 2022New Constraints on Protoplanetary Disk Gas Masses in LupusAug 8, 2019Systematic Variations of CO Gas Abundance with Radius in Gas-rich Protoplanetary DisksAug 6, 2018Transport of CO in Protoplanetary Disks: Consequences of Pebble Formation, Settling, and Radial DriftJun 22, 2020An evolutionary study of volatile chemistry in protoplanetary disksSep 13, 2021Molecules with ALMA at Planet-forming Scales (MAPS) IV: Emission Surfaces and Vertical Distribution of MoleculesSep 13, 2021Molecules with ALMA at Planet-forming Scales (MAPS) XII: Inferring the C/O and S/H ratios in Protoplanetary Disks with Sulfur MoleculesMar 28, 2016The Radial Distribution of H2 and CO in TW Hya as Revealed by Resolved ALMA Observations of CO IsotopologuesJan 20, 2016On the Commonality of 10-30AU Sized Axisymmetric Dust Structures in Protoplanetary DisksSep 13, 2021Molecules with ALMA at Planet-forming Scales (MAPS) II: CLEAN Strategies for Synthesizing Images of Molecular Line Emission in Protoplanetary DisksSep 13, 2021Molecules with ALMA at Planet-forming Scales (MAPS) XVII: Determining the 2D Thermal Structure of the HD 163296 DiskSep 13, 2021Molecules with ALMA at Planet-forming Scales. XX. The Massive Disk Around GM AurigaeSep 13, 2021Molecules with ALMA at Planet-forming Scales (MAPS) V: CO gas distributionsSep 13, 2021Molecules with ALMA at Planet-forming Scales (MAPS). IX. Distribution and Properties of the Large Organic Molecules HC$_3$N, CH$_3$CN, and $c$-C$_3$H$_2$Sep 14, 2021Molecules with ALMA at Planet-forming Scales (MAPS) VI: Distribution of the small organics HCN, C2H, and H2COAug 6, 2018Multiple rings in the transitional disk of GM Aurigae revealed by VLA and ALMAMar 7, 2024Molecular Gas Tracers in Young and Old Protoplanetary DisksFeb 7, 2018Unlocking CO Depletion in Protoplanetary Disks I. The Warm Molecular LayerSep 17, 2024MINDS. JWST-MIRI Observations of a Spatially Resolved Atomic Jet and Polychromatic Molecular Wind Toward SY ChaApr 3, 2026Evidence of Enhanced Ionization in Protostellar Envelopes