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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Main Authors: | , , , , , , , , , , , , , , , , , , , , , |
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Format: | Article |
Language: | English |
Published: |
Maynooth Academic Publishing
2025-06-01
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Series: | The Open Journal of Astrophysics |
Online Access: | https://doi.org/10.33232/001c.140729 |
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