Sánchez-Fernández C.; Kajava J.J.E.; Poutanen J.; Kuulkers E.; Suleimanov V.F.
(2020)
© ESO 2020. Type I X-ray bursts in GS 1826-24, and in several other systems, may induce cooling of the hot inner accretion flow that surrounds the bursting neutron star. Given that GS 1826-24 remained persistently in the ...