Low‐Mass X‐Ray Binaries and Metallicity Dependence: Story of Failures
Low‐Mass X‐Ray Binaries and Metallicity Dependence: Story of Failures
Observations of Galactic and extragalactic globular clusters have shown that, on average, metal-rich clusters are ~3 times more likely to contain a bright X-ray source than their metal-poor counterparts. We propose that this can be explained by taking into account the difference in the stellar structure of main-sequence donors with …