CORDIS Project
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This project aims to enhance our understanding of supernovae and the formation of elements through the study of radio pulsars. By utilizing the advanced LOFAR radio telescope, it seeks to identify stable pulsar systems for direct gravitational wave detection and to test theories of gravity.
A radio pulsar is formed when the iron core of a massive star collapses in a supernova explosion.
Due to their extreme compactness and supernuclear density radio pulsars are extremely stable rotators.
Our goal is 1) to use radio pulsars to improve our limited understanding of some of the most energetic events known in the universe and the source of the elements that make up planets and all forms of life: supernovae 2) to find individual radio-pulsar systems that are such stable rotators that the…
STICHTING ASTRONOMISCH ONDERZOEK IN NEDERLAND
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