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

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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Bibliographic Details
Main Authors:	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
Format:	Article
Language:	English
Published:	Maynooth Academic Publishing 2025-06-01
Series:	The Open Journal of Astrophysics
Online Access:	https://doi.org/10.33232/001c.140729
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Analysis of optical spectroscopy and photometry of the type I X-ray bursting system UW CrB

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