Blazar S5 0716 $$mathbf{+}$ 714：线性极化变化。II

IF 1.3 4区物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS

Astrophysical Bulletin Pub Date : 2024-07-31 DOI:10.1134/S1990341323600370

V. R. Amirkhanyan

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引用次数: 0

摘要

摘要作者在2019-2021年对S5 0716$+$714 进行的线性偏振观测从2021年12月8日持续到2022年3月12日。这些观测结果证实了作者在2022年关于S5 0716$+$714 的线性极化程度与其光通量存在周期性依赖关系的说法。谐波周期在3到55 mJy的区间内从3到8 mJy不等。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

$Blazar S5 0716$\mathbf{+}$714: Linear Polarization Variation. II$

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Blazar S5 0716$\mathbf{+}$714: Linear Polarization Variation. II

The linear polarization observations of S5 0716$+$714 carried out by the author in 2019–2021 were continued from December 8, 2021 to March 12, 2022. These observations confirm the author’s statment made in 2022 about a periodic dependence of the degree of linear polarization of S5 0716$+$714 on its optical flux. The harmonic period varies from 3 to 8 mJy in the 3 to 55 mJy interval.

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来源期刊

Astrophysical Bulletin 地学天文-天文与天体物理

CiteScore

2.00

自引率

33.30%

发文量

审稿时长

>12 weeks

期刊介绍： Astrophysical Bulletin is an international peer reviewed journal that publishes the results of original research in various areas of modern astronomy and astrophysics, including observational and theoretical astrophysics, physics of the Sun, radio astronomy, stellar astronomy, extragalactic astronomy, cosmology, and astronomy methods and instrumentation.