“…6 Thermonuclear X-ray bursts While thermonuclear ('type-I') X-ray bursts are well understood as a thermonuclear runaway in the upper freshly accreted layers of a neutron star in a low-mass X-ray binary, many important questions are unanswered (e.g., Lewin et al, 1993;Strohmayer & Bildsten, 2006;in 't Zand et al, 2015;José, 2016;Galloway & Keek, 2017, see reviews by). Some of those are fundamental, pertaining to the structure of the neutron star and exotic nuclear processes, while others are related to interesting physical phenomena such as neutron star spins, convection and radiation transport under strong-gravity circumstances, the geometry of accretion and magnetic field, and unusual stellar abundances.…”