Refine
Has Fulltext
- yes (1)
Year of publication
- 2012 (1) (remove)
Document Type
- Postprint (1)
Language
- English (1)
Is part of the Bibliography
- yes (1)
Keywords
- X-rays: binaries (1) (remove)
Institute
SXP 1062 is an exceptional case of a young neutron star in a wind-fed high-mass X-ray binary associated with a supernova remnant. A unique combination of measured spin period, its derivative, luminosity and young age makes this source a key probe for the physics of accretion and neutron star evolution. Theoretical models proposed to explain the properties of SXP 1062 shall be tested with new data.