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    Analysis of optical spectroscopy and photometry of the type I X-ray bursting system UW CrB

    Analysis of optical spectroscopy and photometry of the type I X-ray bursting system UW CrB by Mark R. Kennedy, P. Callanan, P. M. Garnavich, R. P. Breton, A. J. Brown, N. Castro Segura, V. S. Dhillon, M. J. Dyer, S. Fijma, J. Garbutt, M. J. Green, P. Hakala, F. Jiminez-Ibarra, P. Kerry, S. Littlefair, J. Munday, P. A. Mason, D. Mata-Sanchez, T. Munoz-Darias, S. Parsons, I. Pelisoli, D. Sahman

    Published 2025-06-01

    UW Coronae Borealis (UW CrB) is a low mass X-ray binary that shows both Type 1 X-ray and optical bursts, which typically last for 20 s. The system has a binary period of close to 2 hours and is thought to have a relatively high inclination due to the presence of an eclipse in the optical light curve...

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