Spiers Memorial Lecture: Astrochemistry at high resolution.
Ceccarelli C.
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Rare earth element nucleosynthetic anomalies and dust transport in the protoplanetary disk. [PDF]
Hu JY +11 more
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Fundamentals of Interior Modelling and Challenges in the Interpretation of Observed Rocky Exoplanets. [PDF]
Baumeister P +9 more
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A 4,565-My-old record of the solar nebula field. [PDF]
Maurel C, Gattacceca J.
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Building wet planets through high-pressure magma-hydrogen reactions. [PDF]
Horn HW +4 more
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Recurrent planetesimal formation in an outer part of the early solar system. [PDF]
Neumann W, Ma N, Bouvier A, Trieloff M.
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A precise metallicity and carbon-to-oxygen ratio for a warm giant exoplanet from its panchromatic JWST emission spectrum. [PDF]
Wiser LS +13 more
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Protoplanetary disks are the places in which planets form around young stars. These environments consist of dust and gas mainly in forms of molecules.Simple and abundant molecules such as water, carbon monoxide, ammonia, play an important role in the disk thermal balance, and allow also observers to study these objects.
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Evidence of the Amino Acids Tyrosine and Phenylalanine in the Interstellar Material of IC348 in Perseus. [PDF]
Iglesias-Groth S +3 more
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A young progenitor for the most common planetary systems in the Galaxy. [PDF]
Livingston JH +41 more
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