activity
20222024
most citedMolecules with ALMA at Planet-forming Scales (MAPS). A Circumplanetary Disk Candidate in Molecular Line Emission in the AS 209 Disk

64 citations · 160 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2024

Multi-Observatory Research of Young Stellar Energetic Flares (MORYSEF): X-ray Flare Related Phenomena and Multi-epoch Behavior

Konstantin V. Getman, Eric D. Feigelson, Abygail R. Waggoner +8

The most powerful stellar flares driven by magnetic energy occur during the early pre-main sequence (PMS) phase. The Orion Nebula represents the nearest region populated by young s…

astro-ph.EP2024

Volatile composition of the HD 169142 disk and its embedded planet

Luke Keyte, Mihkel Kama, Alice S. Booth +2

The composition of a planet's atmosphere is intricately linked to the chemical makeup of the protoplanetary disk in which it formed. Determining the elemental abundances from key v…

astro-ph.EP20241 cited

JWST ice band profiles reveal mixed ice compositions in the HH 48 NE disk

Jennifer B. Bergner, J. A. Sturm, Elettra L. Piacentino +19

Planet formation is strongly influenced by the composition and distribution of volatiles within protoplanetary disks. With JWST, it is now possible to obtain direct observational c…

astro-ph.EP2024

Measuring the and isotopic ratios of volatile sulfur during planet formation

Alice S. Booth, Maria N. Drozdovskaya, Milou Temmink +9

Stable isotopic ratios constitute powerful tools for unraveling the thermal and irradiation history of volatiles. In particular, we can use our knowledge of the isotopic fractionat…

astro-ph.EP2024

Detection of Dimethyl Ether in the Central Region of the MWC 480 Protoplanetary Disk

Yoshihide Yamato, Yuri Aikawa, Viviana V. Guzmán +9

Characterizing the chemistry of complex organic molecules (COMs) at the epoch of planet formation provides insights into the chemical evolution of the interstellar medium (ISM) and…

astro-ph.EP2024

Outflow Driven by a Protoplanet Embedded in the TW Hya Disk

Tomohiro C. Yoshida, Hideko Nomura, Charles J. Law +4

Gas giant planets are formed by gas accretion onto planetary cores in protoplanetary disks. However, direct evidence of this process is still lacking, limiting our understanding of…