电邮这篇文章 METHOD FOR DETERMINING THE PARAMETERS OF A RING-LIKE STRUCTURE FROM THE VISIBILITY FUNCTION SHAPE
- 作者: Chernov S.V.1, Shchurov M.A.1, Bulygin I.I.1, Rudnitskiy A.G.1
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隶属关系:
- Astro Space Center, P. N. Lebedev Physical Institute, Russian Academy of Sciences
- 期: 卷 102, 编号 12 (2025)
- 页面: 1157–1171
- 栏目: Articles
- URL: https://journals.rcsi.science/0004-6299/article/view/361620
- DOI: https://doi.org/10.7868/S3034518925120106
- ID: 361620
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详细
Black hole images obtained by very long baseline interferometry (VLBI) by the Event Horizon Telescope are a new tool for testing general relativity in super-strong gravitational fields. These images demonstrated a ring-like structure which can be explained as the black hole shadow image. To date, there are no reliable methods for determining the parameters of these ring-like structures, such as diameter, width, and asymmetry. In this paper, an algorithm for determining black hole image parameters is proposed using a Gaussian asymmetric ring as an example. Using the proposed method, the diameter and asymmetry parameters of the image of a supermassive black hole in the galaxy M87 were estimated based on observational data obtained by the Event Horizon Telescope group.
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作者简介
S. Chernov
Astro Space Center, P. N. Lebedev Physical Institute, Russian Academy of Sciences
Email: chernov@td.lpi.ru
Moscow, Russia
M. Shchurov
Astro Space Center, P. N. Lebedev Physical Institute, Russian Academy of SciencesMoscow, Russia
I. Bulygin
Astro Space Center, P. N. Lebedev Physical Institute, Russian Academy of SciencesMoscow, Russia
A. Rudnitskiy
Astro Space Center, P. N. Lebedev Physical Institute, Russian Academy of SciencesMoscow, Russia
参考
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