Four infrared-selected young stellar objects are confirmed as FUor eruptions via CO and H2O absorption features, equivalent width diagrams, and disk models showing high extinction and accretion rates comparable to classical FUors.
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JWST spectra of young AB Dor L dwarfs show varying silicate absorption strengths, with 4/5 objects matching the trend of deeper features at equator-on inclinations and a tentative peak-wavelength correlation with viewing angle.
Planet-hosting wide binaries display diverse differential abundance trends with condensation temperature that are not universal across systems.
citing papers explorer
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Characterizing and spectrally modeling embedded FUor eruptions in the near-infrared
Four infrared-selected young stellar objects are confirmed as FUor eruptions via CO and H2O absorption features, equivalent width diagrams, and disk models showing high extinction and accretion rates comparable to classical FUors.
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Clouds with a silicate lining: Using JWST spectra to probe atmospheric diversity in young AB Dor L dwarfs
JWST spectra of young AB Dor L dwarfs show varying silicate absorption strengths, with 4/5 objects matching the trend of deeper features at equator-on inclinations and a tentative peak-wavelength correlation with viewing angle.
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Chemical signatures of planetary systems in their host stars. Near-infrared spectroscopy of four planet-hosting wide binaries
Planet-hosting wide binaries display diverse differential abundance trends with condensation temperature that are not universal across systems.