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The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources

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The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2887705959

The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources

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Ithaca: Cornell University Library, arXiv.org

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Scope and Contents

Contents

Ultraluminous X-ray sources (ULXs) represent an extreme class of accreting compact objects: from the identification of some of the accretors as neutron stars to the detection of powerful winds travelling at 0.1-0.2 c, the increasing evidence points towards ULXs harbouring stellar-mass compact objects undergoing highly super-Eddington accretion. Mea...

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Full title

The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources

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Record Identifier

TN_cdi_proquest_journals_2887705959

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2887705959

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2311.04733

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