Remembering Yury N. Gnedin at the Dawn of X-ray Polarimetry: Predictions of IXPE Observations of Neutron Stars

被引:1
|
作者
Heyl, Jeremy [1 ]
机构
[1] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
magnetars stars; X-rays and stars; star atmospheres; polarization; plasmas; scattering; radiative transfer; STRONGLY MAGNETIZED PLASMA; SURFACE EMISSION; POLARIZATION; RADIATION; FIELD; SCATTERING; EVOLUTION; DISCOVERY; HERCULES; SPECTRA;
D O I
10.3390/universe8020084
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
NASA's Imaging X-ray Polarimetry Explorer (IXPE) was launched in December 2021. It is 100 times more sensitive to polarized X-ray emission than any preceding mission and it is opening a new observational window into high-energy astrophysics. I outline Yury N. Gnedin's many contributions to understanding polarization from neutron stars and present new simulations of observations that IXPE will perform of the X-ray pulsar Hercules X-1 and the magnetar 4U 0141+561 in February 2022. These observations highlight and test particular models that Gnedin and collaborators first proposed. I outline how IXPE will provide unique constraints on the structure and kinematics of the boundary region between the accretion flow and the neutron star surface of Hercules X-1 and how IXPE will verify the predictions of vacuum birefringence for the magnetar 4U 0142+561.
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页数:8
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