Central compact objects and their magnetic fields
arXiv:1210.7112 · doi:10.1017/S1743921312023289
Abstract
Central compact objects (CCOs) are neutron stars that are found near the center of supernova remnants, and their association with supernova remnants indicates these neutron stars are young (<~ 10^4 yr). Here we review the observational properties of CCOs and discuss implications, especially their inferred magnetic fields. X-ray timing and spectral measurements suggest CCOs have relatively weak surface magnetic fields (~ 10^10 - 10^11 G). We argue that, rather than being created with intrinsically weak fields, CCOs are born with strong fields and we are only seeing a weak surface field that is transitory and evolving. This could imply that CCOs are one manifestation in a unified picture of neutron stars.
Proceedings of IAUS 291 "Neutron Stars and Pulsars: Challenges and Opportunities after 80 years", J. van Leeuwen (ed.); 6 pages, 3 figures
References in corpus (11)
- The ATNF Pulsar Catalogue
- Evolution of a buried magnetic field in the central compact object neutron stars
- CCOs and the hidden magnetic field scenario
- Model X-ray Spectra of Magnetic Neutron Stars with Hydrogen Atmospheres
- Discovery of a 112 ms X-ray Pulsar in Puppis A: Further Evidence of Neutron Stars Weakly Magnetized at Birth
- The Hidden Magnetic Field of The Young Neutron Star in Kesteven 79
- The Proper Motion of the Central Compact Object RX J0822-4300 in the Supernova Remnant Puppis A
- Constraining the Geometry of the Neutron Star RX J1856.5-3754
- X-ray Timing of PSR J1852+0040 in Kesteven 79: Evidence of Neutron Stars Weakly Magnetized at Birth
- Magnetized neutron star atmospheres: beyond cold plasma approximation
- A time-variable, phase-dependent emission line in the X-ray spectrum of the isolated neutron star RX J0822-4300
Cited by in corpus (3)
- Tests of the nuclear equation of state and superfluid and superconducting gaps using the Cassiopeia A neutron star
- Diffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron star
- An Overview of Compact Star Populations and Some of Its Open Problems