Sokolova-Lapa E.; Gornostaev M.; Wilms J.; Ballhausen R.; Falkner S.; Postnov K.; Thalhammer P.; Fürst F.; García J.A.; Shakura N.; Becker P.A.; Wolff M.T.; Pottschmidt K.; Härer L.; Malacaria C.
(2021)
Recent observations of X-ray pulsars at low luminosities allow, for the first time, the comparison of theoretical models of the emission from highly magnetized neutron star atmospheres at low mass-accretion rates (M ≤ 1015 ...