MESA simulations show that winds from Type I X-ray bursts igniting at column depths ≥5×10^8 g cm^{-2} eject ash enriched in intermediate-mass to iron-peak elements, with composition depending on ignition depth, accretion mix, and convective treatment.
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Observations show a long thermonuclear burst in MAXI J0911--655 followed by a flare interpreted as burst-driven thermal-viscous disk instability enhancing accretion.
citing papers explorer
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Composition of Radiation-Driven Winds from Type I X-ray Bursts
MESA simulations show that winds from Type I X-ray bursts igniting at column depths ≥5×10^8 g cm^{-2} eject ash enriched in intermediate-mass to iron-peak elements, with composition depending on ignition depth, accretion mix, and convective treatment.
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Long thermonuclear burst driven thermal-viscous instability of accretion disk: triggering an outburst-like X-ray flare
Observations show a long thermonuclear burst in MAXI J0911--655 followed by a flare interpreted as burst-driven thermal-viscous disk instability enhancing accretion.