Unveiling the disc structure in ultraluminous X-ray source NGC 55 ULX-1
(2022)
Journal Article
Barra, F., Pinto, C., Walton, D., Kosec, P., D’Aì, A., Di Salvo, T., Del Santo, M., Earnshaw, H., Fabian, A., Fuerst, F., Marino, A., Pintore, F., Robba, A., & Roberts, T. (2022). Unveiling the disc structure in ultraluminous X-ray source NGC 55 ULX-1. Monthly Notices of the Royal Astronomical Society, 516(3), 3972-3983. https://doi.org/10.1093/mnras/stac2453
Ultraluminous X-ray sources (ULXs) are the most extreme among X-ray binaries in which the compact object, a neutron star or a black hole, accretes matter from the companion star, and exceeds a luminosity of 1039 ergs−1 in the X-ray energy band alone.... Read More about Unveiling the disc structure in ultraluminous X-ray source NGC 55 ULX-1.