New JWST spectra identify C3 as the carrier of the 5.2 um band, detect CS and HCN, link most changes to pulsation, and suggest some prior weak SiC dust reports may be spurious.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 4representative citing papers
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.
A multimodal neural network trained on MPA-JHU references produces SFR, stellar mass, and metallicity estimates for 547 million low-redshift galaxies in DESI LS DR10.
Mid-IR light curves of IRAS20126+4104 confirm a 6.8 yr periodic variation interpreted as evidence that the 12 solar-mass protostar is bloated to a radius of roughly 200 solar radii due to rotation with an obscuring spot.
citing papers explorer
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Mid-infrared JWST spectra of carbon stars in the Large Magellanic Cloud
New JWST spectra identify C3 as the carrier of the 5.2 um band, detect CS and HCN, link most changes to pulsation, and suggest some prior weak SiC dust reports may be spurious.
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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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A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
A multimodal neural network trained on MPA-JHU references produces SFR, stellar mass, and metallicity estimates for 547 million low-redshift galaxies in DESI LS DR10.
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Evidence for a bloated massive protostar in IRAS20126+4104
Mid-IR light curves of IRAS20126+4104 confirm a 6.8 yr periodic variation interpreted as evidence that the 12 solar-mass protostar is bloated to a radius of roughly 200 solar radii due to rotation with an obscuring spot.