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Table · dataset · 2024

JWST MIRI spectrum of T Cha

Listed in IVOA Registry (Virtual Observatory)

Understanding when and how circumstellar disks disperse is crucial to constrain planet formation and migration.

Description

Thermal winds powered by high-energy stellar photons have long been theorized to drive disk dispersal. However, evidence for these winds is currently based only on small (~3-6km/s) blueshifts in [NeII] 12.81{mu}m lines, which does not exclude MHD winds.

We report JWST MIRI MRS spectro-imaging of TCha, a disk with a large dust gap (~30au in radius) and blueshifted [NeII] emission. We detect four forbidden noble gas lines, [ArII], [ArIII], [NeII], and [NeIII], of which [ArIII] is the first detection in any protoplanetary disk. We use line flux ratios to constrain the energy of the ionizing photons and find that argon is ionized by extreme ultraviolet, whereas neon is most likely ionized by X-rays.

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After performing continuum and point-spread function subtraction on the integral field unit cube, we discover a spatial extension in the [NeII] emission off the disk continuum emission. This is the first spatially resolved [NeII] disk wind emission. The mostly ionic spectrum of TCha, in combination with the extended [NeII] emission, points to an evolved stage for any inner MHD wind and is consistent with the existence of an outer thermal wind ionized and driven by high-energy stellar photons.

This work acts as a pathfinder for future observations aiming at investigating disk dispersal using JWST.

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Where it is published

Documentation and papers

Catalogue records · 2

Topics

Stated by source
Infrared
Inferred from text
Astronomical sciences 71%
Provenance · 1 source records, 9 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/aj/167/12714 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (71%)
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:infraredsource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0