The diverse chemistry of protoplanetary disks as revealed by JWST

Author:

van Dishoeck Ewine F.12ORCID,Grant S.2ORCID,Tabone B.3ORCID,van Gelder M.1ORCID,Francis L.1,Tychoniec L.4,Bettoni G.2ORCID,Arabhavi A. M.5ORCID,Gasman D.6ORCID,Nazari P.1ORCID,Vlasblom M.1ORCID,Kavanagh P.7,Christiaens V.8ORCID,Klaassen P.9,Beuther H.10ORCID,Henning Th.10ORCID,Kamp I.5ORCID

Affiliation:

1. Leiden Observatory, Leiden University, P. O. Box 9513, 2300 RA Leiden, The Netherlands

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

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

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

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

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

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

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

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

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

Abstract

Early results from JWST-MIRI programs on low- and high-mass protostars and disks show significant diversity in their mid-infrared spectra, most notably for CO2, H2O and C2H2. Benzene is detected in disks around very low mass stars.

Funder

Nederlandse Organisatie voor Wetenschappelijk Onderzoek

Deutsche Forschungsgemeinschaft

Danmarks Grundforskningsfond

Fonds Wetenschappelijk Onderzoek

H2020 European Research Council

Marie Sklodowska-Curie Actions

Belgian Federal Science Policy Office

Centre National d’Etudes Spatiales

Science and Technology Facilities Council

UK Space Agency

Publisher

Royal Society of Chemistry (RSC)

Subject

Physical and Theoretical Chemistry

Reference138 articles.

1. A rich hydrocarbon chemistry and high C to O ratio in the inner disk around a very low-mass star

2. Astrochemistry and compositions of planetary systems

3. E. F.van Dishoeck and E. A.Bergin , ExoFrontiers; Big Questions in Exoplanetary Science , IOP , Bristol, UK , 2021 , pp. 14–1

4. A.Miotello , I.Kamp , T.Birnstiel , L. I.Cleeves and A.Kataoka , arXiv , 2022 , e-prints, arXiv:2203.09818

5. Temperature Structures of Embedded Disks: Young Disks in Taurus Are Warm

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