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Recent results from cosmic X-ray observations are reviewed, with focus on neutron stars. Properties of three types of these objects are described, based on the results from the Suzaku X-ray observatory. A brief introduction is given to its successor, ASTRO-H, to be launched in 2014.doi:10.1063/1.4763390 fatcat:fkudoxedq5d7jpqajyvzvd5bfy