activity
20182026
most citedMolecules with ALMA at Planet-forming Scales (MAPS) I: Program Overview and Highlights

288 citations · 840 across the 32 of their papers we have counts for

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Showing astro-ph.EPShow all

26 papers · 1 filter

astro-ph.EP2026

JWST-MIRI's multi-dimensional view of mass loss in the irradiated disks of NGC 1977

Alice S. Booth, Qijia Zhou, Jinyoung Serena Kim +10

The evolution of protoplanetary disks, and consequently the outcomes of planet formation, are thought to be significantly altered in regions containing massive stars. Extreme cases…

astro-ph.EP2026★ 3 cited

HO in the terrestrial planet-forming regions of protoplanetary disks

Colette Salyk, Klaus M. Pontoppidan, Ke Zhang +12

Isotopologues play an important role in solar system cosmochemistry studies, revealing details of early planet formation physics and chemistry. Oxygen isotopes, as measured in sola…

astro-ph.EP2025

The chemical diversity of giant-planet nurseries as revealed by ALMA

Alice S. Booth, Jenny Calahan, Milou Temmink +9

With the giant exoplanet occurrence rate peaking around stars of 1.5-2 solar masses, there is strong motivation to characterize the disks that set their formation conditions. Obser…

astro-ph.EP2025

The Impact of External Radiation on the Inner Disk Chemistry of Planet Formation

Jenny K. Calahan, Karin Öberg, Alice Booth

The vast majority of young stars hosting planet-forming disks exist within clustered environments, like the Orion Nebula, implying that seemingly `extreme' UV environments (10^4 G_…

astro-ph.EP2025

Ice sublimation in the dynamic HD 100453 disk reveals a rich reservoir of inherited complex organics

Alice S. Booth, Lisa Wölfer, Milou Temmink +7

Protoplanetary disks around luminous young A-type stars are prime observational laboratories to determine the abundances of complex organic molecules (COMs) present during planet f…

astro-ph.EP2024

JWST/MIRI detection of a carbon-rich chemistry in a solar nebula analog

Maria Jose Colmenares, Edwin Bergin, Colette Salyk +16

It has been proposed, and confirmed by multiple observations, that disks around low mass stars display a molecule-rich emission and carbon-rich disk chemistry as compared to their…