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An ultraluminous X-ray source powered by an accreting neutron star.

NATURE, no. 7521 (2014): 202-+

Cited: 284|Views7

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pubmed.ncbi.nlm.nih.gov arxiv.org

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High-energy astrophysics

Abstract

The majority of ultraluminous X-ray sources are point sources that are spatially offset from the nuclei of nearby galaxies and whose X-ray luminosities exceed the theoretical maximum for spherical infall (the Eddington limit) onto stellar-mass black holes(1,2). Their X-ray luminosities in the 0.5-10 kiloelectronvolt energy band range from...More

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