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Using a novel binary population synthesis code, we investigate the evolutionary pathways that can transform main sequence binaries into a HMXB phase.
We also derive scaling relations between the number of X-ray binaries and the star-formation rate and stellar mass, and we compare them with results from X-ray binary population synthesis models.
In turn, the updated multiplicity statistics serve as more reliable initial conditions in binary population synthesis studies of Type Ia supernovae, X-ray binaries, and sources of gravitational waves.
We propose a deep (4 x 75ksec) ACIS-S observation to measure the complete populations of millisecond pulsars (MSPs) and cataclysmic variables (CVs) by their variability and spectra and to constrain the main sequence binary population.
We show several key results including a connection between electron-capture supernovae and the population of Be-HXMBs, and a dynamical model explaining the metallicity dependence of the ultra-luminous X-Ray binary population.
Statistical studies though, offer a chance to study the ULXs as a class through (i) the connection of the populations with the bulk properties of the host galaxies, and (ii) the comparison with binary population synthesis studies.
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The X-ray evolution of the luminosity of normal galaxies is primarily driven by the evolution of their X-ray binary populations.
Finally, we present the first results from a study of a sample of nearby star-forming galaxies which form a starburst age sequence: although their XLFs to first order are represented by power-laws with consistent slopes, there is an indication for small variations, suggesting a change of their X-ray binary populations.
Our incomplete understanding of the stability of mass transfer leads to differences between synthetic binary populations (Toonen et al. 2014).
Google also recognizes its gender reporting is "not inclusive of our non-binary population" and is looking for the best way to measure gender moving forward.
In young starburst galaxies, the relics of the most short-lived and hence most massive stars could dominate the X-ray binary (XRB) population.
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com