Super-Resolved Image of M87 Observed with East Asian VLBI Network

IF 3.2 Q2 ASTRONOMY & ASTROPHYSICS
Galaxies Pub Date : 2023-02-28 DOI:10.3390/galaxies11020039
F. Tazaki, Yuzhu Cui, K. Hada, M. Kino, I. Cho, Guangyao Zhao, K. Akiyama, Y. Mizuno, H. Ro, M. Honma, R. Lu, Zhi-qiang Shen, L. Cui, Y. Yonekura
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引用次数: 0

Abstract

Obtaining high-resolution images at centimeter-or-longer wavelengths is vital for understanding the physics of jets. We reconstructed images from the M87 22 GHz data observed with the East Asian VLBI Network (EAVN) by using the regularized maximum likelihood (RML) method, which is different from the conventional imaging method CLEAN. Consequently, a bright core and jet extending about 30 mas to the northwest were detected with a higher resolution than in the CLEAN image. The width of the jet was 0.5 mas at 0.3 mas from the core, consistent with the width measured in the 86 GHz image in the previous study. In addition, three ridges were able to be detected at around 8 mas from the core, even though the peak-to-peak separation was only 1.0 mas. This indicates that the RML image’s spatial resolution is at least 30% higher than that of the CLEAN image. This study is an important step for future multi-frequency and high-cadence observations of the EAVN to discuss the more detailed structure of the jet and its time variability.
东亚VLBI网络观测M87的超分辨图像
获得厘米或更长波长的高分辨率图像对于理解喷流的物理特性至关重要。我们使用正则化最大似然(RML)方法从东亚VLBI网络(EAVN)观测到的M87 22GHz数据中重建图像,该方法不同于传统的成像方法CLEAN。因此,以比CLEAN图像中更高的分辨率检测到了向西北方向延伸约30mas的明亮核心和喷流。在距离核心0.3 mas处,喷流的宽度为0.5 mas,与之前研究中在86 GHz图像中测量的宽度一致。此外,尽管峰间分离仅为1.0mas,但在距离核心约8mas时仍能检测到三个脊。这表明RML图像的空间分辨率至少比CLEAN图像高30%。这项研究是未来对EAVN进行多频率和高节奏观测的重要一步,以讨论更详细的喷流结构及其时间可变性。
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来源期刊
Galaxies
Galaxies Physics and Astronomy-Astronomy and Astrophysics
CiteScore
4.90
自引率
12.00%
发文量
100
审稿时长
11 weeks
期刊介绍: Es una revista internacional de acceso abierto revisada por pares que proporciona un foro avanzado para estudios relacionados con astronomía, astrofísica y cosmología. Areas temáticas Astronomía Astrofísica Cosmología Astronomía observacional: radio, infrarrojo, óptico, rayos X, neutrino, etc. Ciencia planetaria Equipos y tecnologías de astronomía. Ingeniería Aeroespacial Análisis de datos astronómicos. Astroquímica y Astrobiología. Arqueoastronomía Historia de la astronomía y cosmología. Problemas filosóficos en cosmología.
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