SIMBAD references

2025RNAAS...9..316H - Research Notes of the AAS, 9, 316 (2025/November-0)

A New FU Orionis Accretion Outburst in the W5 H II Region.

HILLENBRAND L.A., GRAHAM M.J., KASLIWAL M.M., PURDUM J., SOLLERMAN J., CARVALHO A.S., KUHN M.A., SMITH R., ASHLEY M.C.B., EARLEY N., LAHER R.R. and CHEN T.X.

Abstract (from CDS):

We announce a recently detected outburst that is currently only a few months old, and probably of FU Orionis type. The progenitor to the outburst was an emission-line, flat-spectrum spectral energy distribution young stellar object located in the W5 region, though somewhat outside the main star formation action. We present optical, near-infrared, and mid-infrared lightcurves that illustrate the quiescent state of [KAG2008] 13656 and its subsequent Δr ≈ -4 mag and ΔJ ≈ -3 mag outburst over ∼75 days in late-2025. Follow-up optical and near-infrared spectroscopy confirms the expected features from an FU Ori disk and outflow.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): FU Orionis stars - Young stellar objects

Simbad objects: 2

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