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中央研究院天文及天文物理研究所
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研究成果藝廊 > 特長基線干涉儀

研究成果藝廊

特長基線干涉儀

First Polarization Image around the Black Hole Shadow
圖片來源: EHT Collaboration
First Polarization Image around the Black Hole Shadow
The polarized light at the vicinity of the black hole for the first time (EHT Collaboration et al. 2021, ApJL, 910, L12), which carries the magnetic field and plasma information very close to the black hole.
The maximum linear polarization fraction reaches up to ~15%, and the net azimuthal linear polarization pattern may result from organized, poloidal magnetic fields. In addition, through the general relativistic magnetohydrodynamic (GRMHD) simulations, we infer the mass accretion rate onto the black hole in M87 as (3-20) x 10^-4 Mo/yr (EHT Collaboration et al. 2021, ApJL, 910, L13).
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