Understanding radio pulsars using modern broad-band instruments
<p>The canonical model of a pulsar is insufficient to describe the variety and variability of its radio emission. Pulsars are neutron stars, with intense gravitational and magnetic fields, which emit bright beams of radio waves that co-rotate with the spinning star. The regularity of pulsar ro...
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| Muut tekijät: | |
| Aineistotyyppi: | Opinnäyte |
| Kieli: | English |
| Julkaistu: |
2021
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| Aiheet: |