Fast X-ray transients shine light on how stars end their lives and the distant universe
A new kind of stellar explosion provides a novel way to probe the distant universe, according to new results published today in Nature Astronomy.
Stars, as physical systems, are self-gravitating, approximately hydrostatic spheres of plasma in which energy is generated predominantly by thermonuclear fusion in their cores and transported outward by radiation and/or convection. Their structure is governed by the equations of stellar structure, balancing gravity, gas and radiation pressure, and energy transport. Stellar properties such as mass, composition, and rotation determine their internal stratification, nucleosynthetic pathways, luminosity, temperature, and evolutionary tracks. Stars interact with their environments via radiation, stellar winds, and mass loss, and they serve as fundamental sites of element synthesis and key components of galactic and cosmological structure.
A new kind of stellar explosion provides a novel way to probe the distant universe, according to new results published today in Nature Astronomy.
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