Retrieval of Thermally Resolved Water Vapor Distributions in Disks Observed with JWST-MIRI

The mid-infrared water vapor emission spectrum provides a novel way to characterize the delivery of icy pebbles toward the innermost (<5 au) regions of planet-forming disks. Recently, JWST MIRI-MRS showed that compact disks exhibit an excess of low-energy water vapor emission relative to extended...

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Bibliographic Details
Published in:The Astrophysical Journal
Main Authors: Carlos E. Romero-Mirza, Andrea Banzatti, Karin I. Öberg, Klaus M. Pontoppidan, Colette Salyk, Joan Najita, Geoffrey A. Blake, Sebastiaan Krijt, Nicole Arulanantham, Paola Pinilla, Feng Long, Giovanni Rosotti, Sean M. Andrews, David J. Wilner, Jenny Calahan, The JDISCS Collaboration
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Subjects:
Protoplanetary disks
Planet formation
Water vapor
James Webb Space Telescope
Astrochemistry
Infrared spectroscopy
Online Access:https://doi.org/10.3847/1538-4357/ad769e

Internet

https://doi.org/10.3847/1538-4357/ad769e

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