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(1 - 20 of 21)

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The chemical inventory of the inner regions of planet-forming disks - the JWST/MINDS program
MINDS. The detection of ^13CO_2 with JWST-MIRI indicates abundant CO_2 in a protoplanetary disk
Evidence for ubiquitous carbon grain destruction in hot protostellar envelopes
How large Is a disk-what do protoplanetary disk gas sizes really mean?
A rich hydrocarbon chemistry and high C to O ratio in the inner disk around a very low-mass star
Water in the terrestrial planet-forming zone of the PDS 70 disk
Formation of the methyl cation by photochemistry in a protoplanetary disk
OH mid-infrared emission as a diagnostic of H2O UV photodissociation
A major asymmetric ice trap in a planet-forming disk
Importance of source structure on complex organics emission
Directly tracing the vertical stratification of molecules in protoplanetary disks
MINDS
Constraining turbulence in protoplanetary discs using the gap contrast: an application to the DSHARP sample
The diverse chemistry of protoplanetary disks as revealed by JWST
The distribution of accretion rates as a diagnostic of protoplanetary disc evolution
Experimental and theoretical needs for the JWST Early Release Science Program on radiative feedback from massive stars (PDRs4ALL)
Experimental and theoretical needs for the JWST Early Release Science Program PDRs4All: radiative feedback from massive stars
N-bearing complex organics toward high-mass protostars
Importance of source structure on complex organics emission. I.
Modelling the secular evolution of protoplanetary disc dust sizes

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