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.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.HE 3years
2026 3verdicts
UNVERDICTED 3representative citing papers
Observations show a long thermonuclear burst in MAXI J0911--655 followed by a flare interpreted as burst-driven thermal-viscous disk instability enhancing accretion.
XSPECT observations of two soft X-ray transients during outburst decay reveal superburst evolution with cooling blackbody emission and a flux-dependent hardening of Comptonized spectra.
citing papers explorer
-
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.
-
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.
-
Tracing the outburst decay of soft X-ray transients Aql X-1 and 4U 1608-52 with XSPECT
XSPECT observations of two soft X-ray transients during outburst decay reveal superburst evolution with cooling blackbody emission and a flux-dependent hardening of Comptonized spectra.