The diverse chemistry of protoplanetary disks as revealed by JWST.


Journal

Faraday discussions
ISSN: 1364-5498
Titre abrégé: Faraday Discuss
Pays: England
ID NLM: 9212301

Informations de publication

Date de publication:
20 Sep 2023
Historique:
medline: 27 6 2023
pubmed: 27 6 2023
entrez: 27 6 2023
Statut: epublish

Résumé

Early results from the James Webb Space Telescope-Mid-InfraRed Instrument (JWST-MIRI) guaranteed time programs on protostars (JOYS) and disks (MINDS) are presented. Thanks to the increased sensitivity, spectral and spatial resolution of the MIRI spectrometer, the chemical inventory of the planet-forming zones in disks can be investigated with unprecedented detail across stellar mass range and age. Here, data are presented for five disks, four around low-mass stars and one around a very young high-mass star. The mid-infrared spectra show some similarities but also significant diversity: some sources are rich in CO

Identifiants

pubmed: 37366333
doi: 10.1039/d3fd00010a
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

52-79

Auteurs

Ewine F van Dishoeck (EF)

Leiden Observatory, Leiden University, P. O. Box 9513, 2300 RA Leiden, The Netherlands. ewine@strw.leidenuniv.nl.
Max-Planck Institut für Extraterrestrische Physik (MPE), Giessenbachstr. 1, 85748, Garching, Germany.

S Grant (S)

Max-Planck Institut für Extraterrestrische Physik (MPE), Giessenbachstr. 1, 85748, Garching, Germany.

B Tabone (B)

Université Paris-Saclay, CNRS, Institut d'Astrophysique Spatiale, 91405, Orsay, France.

M van Gelder (M)

Leiden Observatory, Leiden University, P. O. Box 9513, 2300 RA Leiden, The Netherlands. ewine@strw.leidenuniv.nl.

L Francis (L)

Leiden Observatory, Leiden University, P. O. Box 9513, 2300 RA Leiden, The Netherlands. ewine@strw.leidenuniv.nl.

L Tychoniec (L)

European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching bei München, Germany.

G Bettoni (G)

Max-Planck Institut für Extraterrestrische Physik (MPE), Giessenbachstr. 1, 85748, Garching, Germany.

A M Arabhavi (AM)

Kapteyn Astronomical Institute, Rijksuniversiteit Groningen, P. O. Box 800, 9700 AV Groningen, The Netherlands.

D Gasman (D)

Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium.

P Nazari (P)

Leiden Observatory, Leiden University, P. O. Box 9513, 2300 RA Leiden, The Netherlands. ewine@strw.leidenuniv.nl.

M Vlasblom (M)

Leiden Observatory, Leiden University, P. O. Box 9513, 2300 RA Leiden, The Netherlands. ewine@strw.leidenuniv.nl.

P Kavanagh (P)

Dublin Institute for Advanced Studies, Astronomy & Astrophysics Section, 31 Fitzwilliam Place, Dublin 2, Ireland.

V Christiaens (V)

STAR Institute, Université de Liège, Allée du Six Août 19c, 4000 Liège, Belgium.

P Klaassen (P)

UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ, UK.

H Beuther (H)

Max-Planck-Institut für Astronomie (MPIA), Königstuhl 17, 69117 Heidelberg, Germany.

Th Henning (T)

Max-Planck-Institut für Astronomie (MPIA), Königstuhl 17, 69117 Heidelberg, Germany.

I Kamp (I)

Kapteyn Astronomical Institute, Rijksuniversiteit Groningen, P. O. Box 800, 9700 AV Groningen, The Netherlands.

Classifications MeSH