Polarization Properties of Energetic Pulsars at Meterwavelengths
Polarization behavior shows a transition in the pulsar population, where energetic sources with higher spin-down energy loss, $\dot{E}\gt 1{0}^{34}$ erg s ^−1 , often have fractional linear polarization ( L / I ) close to 100%, while below this range L / I is usually lower than 50%. The polarization...
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| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/addab1 |
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