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Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925

Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2632509794

Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925

About this item

Full title

Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2022-02

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Variability is a powerful tool to investigate properties of X-ray binaries (XRB), in particular for Ultraluminous X-ray sources (ULXs) that are mainly detected in the X-ray band. For most ULXs the nature of the accretor is unknown, although a few ULXs have been confirmed to be accreting at super-Eddington rates onto a neutron star (NS). Monitoring...

Alternative Titles

Full title

Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2632509794

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2632509794

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2202.11158

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