Central Compact Objects in Supernova Remnants

Abstract

Central Compact Objects (CCOs) are a handful of sources located close to the geometrical center of young supernova remnants. They only show thermal-like, soft X-ray emission and have no counterparts at any other wavelength. While the first observed CCO turned out to be a very peculiar magnetar, discovery that three members of the family are weakly magnetised Isolated Neutron Stars (INSs) set the basis for an interpretation of the class. However, the phenomeology of CCOs and their relationship with other classes of INSs, possibly ruled by supernova fall-back accretion, are still far from being well understood.

7 pages, to appear in the proceedings of "Physics of Neutron Stars - 2017" Conference (July 10-14, Saint Petersburg), JPCS, eds. G.G. Pavlov, J.A. Pons, P.S. Shternin & D.G. Yakovlev

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• Central Compact Objects in Supernova Remnants
• Discovery of an Isolated Compact Object at High Galactic Latitude
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Cited by in corpus (26)

• Magnetic, thermal and rotational evolution of isolated neutron stars
• Science objectives of the Einstein Probe mission
• NS 1987A in SN 1987A
• Diffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron star
• Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A
• Do Central Compact Objects have Carbon Atmospheres?
• A Search for Late-Time Radio Emission and Fast Radio Bursts from Superluminous Supernovae
• Powering Central Compact Objects with a Tangled Crustal Magnetic Field
• Deep infrared observations of the puzzling central X-ray source in RCW103
• Discovery of a very young high-mass X-ray binary associated with the supernova remnant MCSNRJ0513-6724 in the LMC
• X-ray bounds on cooling, composition, and magnetic field of the Cassiopeia A neutron star and young central compact objects
• 3D Magneto-thermal Simulations of Tangled Crustal Magnetic Field in Central Compact Objects
• The Proper Motion of the Central Compact Object RX J0822-4300 in the Supernova Remnant Puppis A, Revisited
• Magnetic Field Evolution in Neutron Star Crusts: Beyond the Hall Effect
• A kinematic study of central compact objects and their host supernova remnants
• Thermal and non-thermal X-ray emission from the rotation-powered radio/$\gamma$-ray pulsar PSR J1740+1000
• Neutron Star Interior Composition Explorer X-ray Timing of the Radio and Gamma-ray Quiet Pulsars PSR J1412+7922 AND PSR J1849-0001
• Constraints on neutron star superfluidity from the cooling neutron star in Cassiopeia A using all Chandra ACIS-S observations
• A LOFAR search for steep-spectrum pulsars in Supernova Remnants and Pulsar Wind Nebulae
• Tracking the footprints of the radio pulsar B1727$-$47: proper motion, host supernova remnant, and the glitches
• An Overview of Compact Star Populations and Some of Its Open Problems
• Magnetic field sustained by the elastic force in neutron star crusts
• Measuring the Non-Axially-Symmetric Surface Temperature Distribution of the Central Compact Object in Puppis A
• Expected polarization properties of nonmagnetized CCOs
• Strongly pulsed thermal X-rays from a single extended hot spot on PSR J2021+4026
• TRAPUM upper limits on pulsed radio emission for SMC X-ray pulsar J0058-7218