Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the Small Magellanic Cloud (2014)
Attributed to:
Modelling compact objects for precision astrophysics
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stt2192
Publication URI: http://dx.doi.org/10.1093/mnras/stt2192
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 4