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The Magnificent Seven: Nearby Isolated Neutron Stars with strong Magnetic Fields

F. Haberl
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Abstract

Although the true origin of the broad absorption lines in X-ray spectra of thermal isolated neutron stars is not clear yet, our current knowledge about the "magnificent seven" strongly suggests that they are highly magnetized ($10^{13} - 10^{14}$ G), slowly rotating cooling neutron stars. Further timing studies would be very useful to obtain more independent estimates of the magnetic field strength (as they currently only exist from RX J0720.4-3125).

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F. Haberl. 2005-10-17. The Magnificent Seven: Nearby Isolated Neutron Stars with strong Magnetic Fields. https://arxiv.org/abs/astro-ph/0510480

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