... of stable configurations, with systems found to orbit around stars with different ages, including binaries and even pulsars. Nevertheless, multiple planetary systems around evolved giants, appear to account for a very small fraction of the planets...
... burst radio afterglow, and that its existence and timescale was not in line with originating from a pulsar or supernovae. As the team were able to measure the redshift of the burst along with its dispersion signal...
... stemming from technogenic factors and sun radiation; cosmic radiation from nuclear reactions in novae, supernovae and pulsars; and the danger of Earth infection by microorganisms from meteors and other small celestial bodies. The third...
... at the turbulent and extreme environments of phenomena such as stellar and supermassive black holes, neutron stars and pulsars. The one thing these objects have in common is an abundance of high energy X-ray radiation and clues to the...
... measure the stars' properties. The astronomers are then able to locate various objects and events, including pulsars or explosions. The Cambridge team used Gaia data to study the Magellanic Clouds and locate RR Lyrae stars...
... and evolve to produce the myriad of exoplanets we see today. Since the first confirmed detection of an exoplanet around a pulsar in 1991, thousands of exoplanets have been discovered and their diversity appears endless. All manner of exoworlds from...