A Spatially Resolved X-Ray Polarization Map of the Vela Pulsar Wind Nebula

Abstract In this paper, we present a full spatially resolved polarization map for the Vela pulsar wind nebula (PWN) observed by IXPE. By employing effective background discrimination techniques, our results show a remarkably high degree of local polarization in the outskirt region, exceeding 60% (55...

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Published inAstrophysical journal. Letters Vol. 959; no. 1; p. L2
Main Authors Liu, Kuan, Xie, Fei, Liu, Yi-han, Ng, Chi-Yung, Bucciantini, Niccolò, Romani, Roger W., Weisskopf, Martin C., Costa, Enrico, Di Marco, Alessandro, La Monaca, Fabio, Muleri, Fabio, Soffitta, Paolo, Deng, Wei, Meng, Yu, Liang, En-wei
Format Journal Article
LanguageEnglish
Published Austin The American Astronomical Society 01.12.2023
IOP Publishing
Subjects
Consistency
Magnetic fields
Nebulae
Polarimetry
Polarization
Pulsar wind nebulae
Pulsar winds
Pulsars
Radio emission
Radio observation
Stellar winds
Supernova
Synchrotrons
Wind
X-ray astronomy
X-rays
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Summary:Abstract In this paper, we present a full spatially resolved polarization map for the Vela pulsar wind nebula (PWN) observed by IXPE. By employing effective background discrimination techniques, our results show a remarkably high degree of local polarization in the outskirt region, exceeding 60% (55%) with a probability of 95% (99%), which approaches the upper limit predicted by the synchrotron emission mechanism. The high degree of polarization suggests that the turbulent magnetic energy is at most 33% of the ordered one. In addition, the X-ray polarization map exhibits a toroidal magnetic field pattern that is consistent with the field revealed by radio observations across the entire nebula. This consistency reveals that the observed X-ray and radio emissions are radiated by electrons from the same magnetic field. Different from the Crab PWN, the consistency observed in the Vela PWN may be attributed to the interaction between the reverse shock of the supernova blast wave and the PWN, which leads to a displacement between the synchrotron-cooled nebula and the fresh nebula close to the pulsar. These findings deepen our understanding of the structure and evolution of the Vela PWN and the magnetohydrodynamic interaction in PWNe.
Bibliography:High-Energy Phenomena and Fundamental Physics
AAS50489
ISSN:2041-8205
2041-8213
DOI:10.3847/2041-8213/ad0bfc