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This volume, the proceedings of IAU Symposium 363, addresses the astrophysical implications of gravitational wave and electromagnetic observations of neutron stars. It covers the …
A new paradigm for scientific discovery through computational tools now permeates every aspect of astronomical research. Computational astrophysics combines modern computational …
The prime parameter determining the evolution of a star is its mass. Any modification to the stellar mass has large repercussions on its evolutionary path. Both low-mass and …
Blazars, the most extreme active galactic nuclei with powerful relativistic jets extending out to kiloparsecs from their central engine, are among the most intriguing and …
Multi-messenger science has a long history in solar astronomy, as direct measures of “in-situ” particles emanating from the Sun, like the solar wind, have long been used alongside …
Winds form an integral part of astronomy – from regulating rotation of stars through enriching galaxies with fresh materials. Outflowing winds persist during the entire lives of …
Star formation is relevant to nearly every area of astrophysics, from planetary science to galaxy evolution, yet the physical processes that determine the rates of star formation …