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Nature|August 24, 2023
Outflows from the youngest stars are mostly molecularT P Ray, M J McCaughrean, A Caratti O Garatti, et al.Chemistry (Weinheim an Der Bergstrasse, Germany)|January 11, 2016
Studies of a Large Odd-Numbered Odd-Electron Metal Ring: Inelastic Neutron Scattering and Muon Spin Relaxation Spectroscopy of Cr8 MnMichael L Baker, Tom Lancaster, Alessandro Chiesa, et al.Science (New York, N.Y.)|February 22, 2024
Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987AC Fransson, M J Barlow, P J Kavanagh, et al.Nature|November 15, 2023
SO<sub>2</sub>, silicate clouds, but no CH<sub>4</sub> detected in a warm NeptuneAchrène Dyrek, Michiel Min, Leen Decin, et al.Science (New York, N.Y.)|June 6, 2024
Abundant hydrocarbons in the disk around a very-low-mass starA M Arabhavi, I Kamp, Th Henning, et al.Faraday Discussions|July 18, 2023
The chemical inventory of the inner regions of planet-forming disks - the JWST/MINDS programInga Kamp, Thomas Henning, Aditya M Arabhavi, et al.Nature|July 24, 2023
Water in the terrestrial planet-forming zone of the PDS 70 diskG Perotti, V Christiaens, Th Henning, et al.Nature|November 29, 2023
A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067R Luque, H P Osborn, A Leleu, et al.Science (New York, N.Y.)|February 12, 2026
Gas-depleted planet formation occurred in the four-planet system around the red dwarf LHS 1903Thomas G Wilson, Anna M Simpson, Andrew Collier Cameron, et al.Pageof 11