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

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

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. Their X-ray luminosities in the 0.5–10 kilo...

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Bibliografiska uppgifter
Huvudupphovsmän: Bachetti, M., Harrison, Fiona A., Walton, D. J., Grefenstette, Brian W., Fürst, F., Barret, D., Beloborodov, A., Boggs, S. E., Christensen, F. E., Craig, W. W., Fabian, A. C., Hailey, Charles J., Hornschemeier, A., Kaspi, Victoria, Kulkarni, S. R., Maccarone, T. J., Miller, J. M., Rana, V., Stern, D., Tendulkar, S. P., Tomsick, J., Webb, N. A., Zhang, W. W., Chakrabarty, Deepto
Övriga upphovsmän: Massachusetts Institute of Technology. Department of Physics
Materialtyp: Artikel
Språk:en_US
Publicerad: Nature Publishing Group 2015
Länkar:http://hdl.handle.net/1721.1/98042
https://orcid.org/0000-0001-8804-8946

Internet

http://hdl.handle.net/1721.1/98042
https://orcid.org/0000-0001-8804-8946

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