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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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.SR 2years
2026 2representative citing papers
SPICY 97589 is an M3 star of 0.29 solar masses whose 2023 outburst was powered by an accretion rate of 2.38e-7 solar masses per year, two orders of magnitude above its quiescent level.
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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Characterisation of an EXor outburst SPICY 97589
SPICY 97589 is an M3 star of 0.29 solar masses whose 2023 outburst was powered by an accretion rate of 2.38e-7 solar masses per year, two orders of magnitude above its quiescent level.