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arXiv · 1711.05038

What will eROSITA reveal among X-ray faint isolated neutron stars?

Adriana Mancini Pires
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Abstract

Since the discovery of the first radio pulsar fifty years ago, the population of neutron stars in our Galaxy has grown to over 2,600. A handful of these sources, exclusively seen in X-rays, show properties that are not observed in normal pulsars. Despite their scarcity, they are key to understanding aspects of the neutron star phenomenology and evolution. The forthcoming all-sky survey of eROSITA will unveil the X-ray faint end of the neutron star population at unprecedented sensitivity; therefore, it has the unique potential to constrain evolutionary models and advance our understanding of the sources that are especially silent in the radio and $\gamma$-ray regimes. In this contribution I discuss the expected role of eROSITA, and the challenges it will face, at probing the galactic neutron star population.

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Adriana Mancini Pires. 2017-11-14. What will eROSITA reveal among X-ray faint isolated neutron stars?. https://arxiv.org/abs/1711.05038

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