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Unveiling the X-ray faint end of the Isolated Neutron Star Population

Unveiling the X-ray faint end of the Isolated Neutron Star Population
揭示孤立中子星群的 X 射线微弱末端
批准号:
448477134
负责人:
Privatdozent Dr. Axel Schwope
金额:
$0.0万
依托单位国家:
德国
项目类别:
Research Units
财政年份:
--
资助国家:
德国
项目状态:
未结题
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中文摘要
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英文摘要
Since the discovery of the first radio pulsar fifty years ago, the population of isolated neutron stars (INSs) in our Galaxy has grown to ∼2800, out of which a few per cent are exclusively seen in X-rays. Despite their scarcity, the X-ray emitting INSs are the key to understanding aspects of neutron star phenomenology and evolution not observed in normal pulsars. eRASS will unveil the X-ray faint end of the population; therefore, it has the unique potential to constrain evolutionary models and advance the understanding of the NS population as a whole.
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