Browsing by Subject "stars: neutron"
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- ItemOpen AccessLong-term evolution of the neutron-star spin period of SXP 1062(2013) Sturm, R; Haberl, F; Oskinova, L M; Schurch, M P E; Hénault-Brunet, V; Gallagher, J S; Udalski, AContext. The Be/X-ray binary SXP 1062 is of especial interest owing to the large spin period of the neutron star, its large spin-down rate, and the association with a supernova remnant constraining its age. This makes the source an important probe for accretion physics.
- ItemOpen AccessLong-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave(2017) Alfonso-Garzón, J; Fabregat, J; Reig, P; Kajava, J J E; Sánchez-Fernández, C; Townsend, L J; Mas-Hesse, J M; Crawford, S M; Kretschmar, P; Coe, M JContext. Multiwavelength monitoring of Be/X-ray binaries is crucial to understand the mechanisms producing their outbursts. H 1145-619 is one of these systems, which has recently displayed X-ray activity.