For most of 47 classical T Tauri stars, the fastness parameter is below equilibrium, implying active angular momentum loss and dynamic star-disk interaction.
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6 Pith papers cite this work, alongside 139 external citations. Polarity classification is still indexing.
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WISE J054452.25+333009.6 is a newly identified FU Orionis outburst, seen nearly face-on, with accretion parameters derived from a disk model.
HL Tau's X-ray spectrum stays hot (about 30 million degrees) across 20 years, with a possible but unconfirmed ~21-day modulation in its 2020 X-ray light curve.
A decade-long infrared survey of Cygnus-X reveals 68 candidate eruptive young stars, with large outbursts roughly ten times more frequent among embedded Class I protostars than among more evolved Class II objects.
Two-epoch medium-band photometry of 769 YSO candidates in Orion A identifies 110 variables (~14%), with best-fit templates dominated by cold and hot spot models over extinction or gray changes.
citing papers explorer
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The ODYSSEUS Survey. Using accretion and stellar rotation to reveal the star-disk connection in T Tauri stars
For most of 47 classical T Tauri stars, the fastness parameter is below equilibrium, implying active angular momentum loss and dynamic star-disk interaction.
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FUOr-Aur 0544+3330: A New YSO Outburst in the Outskirts of Auriga OB1, Viewed Face-On
WISE J054452.25+333009.6 is a newly identified FU Orionis outburst, seen nearly face-on, with accretion parameters derived from a disk model.
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Long-Term X-ray Variability on the Benchmark YSO HL Tau
HL Tau's X-ray spectrum stays hot (about 30 million degrees) across 20 years, with a possible but unconfirmed ~21-day modulation in its 2020 X-ray light curve.
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Eruptive YSOs in Cygnus-X: a mid-infrared variability study with NEOWISE and SPICY
A decade-long infrared survey of Cygnus-X reveals 68 candidate eruptive young stars, with large outbursts roughly ten times more frequent among embedded Class I protostars than among more evolved Class II objects.
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7DT Insight: Variability in Young Stellar Objects
Two-epoch medium-band photometry of 769 YSO candidates in Orion A identifies 110 variables (~14%), with best-fit templates dominated by cold and hot spot models over extinction or gray changes.
- Preparing for the Early eVolution Explorer: Photometric Diagnostics of Magnetospheric Accretion Geometry in Young Stellar Objects