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.
K., Chenevez, J., Strohmayer, T
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Multi-wavelength data classify the Einstein Probe transient EP250916a as a faint hard-state black hole X-ray binary candidate.
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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On The Nature of Einstein Probe Transient EP250916a: Insights from X-ray, Optical, and Radio Observations
Multi-wavelength data classify the Einstein Probe transient EP250916a as a faint hard-state black hole X-ray binary candidate.