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耀变体PKS2155-304的光学波段光变特性

杨海燕 李孝攀 罗玉辉 杨海涛 木繁

云南师范大学学报(自然科学版)2017,Vol.37Issue(6):1-5,5.
云南师范大学学报(自然科学版)2017,Vol.37Issue(6):1-5,5.DOI:10.7699/j.ynnu.ns-2017-070

耀变体PKS2155-304的光学波段光变特性

The Optical Variation of the Blazar Object PKS 2155-304

杨海燕 1李孝攀 1罗玉辉 1杨海涛 1木繁2

作者信息

  • 1. 昭通学院物理与信息工程学院,云南昭通657000
  • 2. 昆明理工大学津桥学院,云南昆明650106
  • 折叠

摘要

Abstract

This paper uses the Swift satellite UVOT telescope observation data to obtain the light curve of PKS 2155-304 on optical U band and B band from November 17,2005 to September 8,2017.Jurkevich method is applied to the light curve,the analysis results show that the PKS 2155-304 on optical U band could have 237 days of quasi periodicity,B band could have 242 days of quasi periodicity.The results are validated by DCF method.The DCF method also found that optical U band and B band were strongly correlated without significant time delay.

关键词

PKS 2155-304/Jurkevich方法/DCF方法/光变周期/相关性

Key words

PKS 2155-304/Jurkevich method/DCF method/Variability period/Correlation

分类

天文与地球科学

引用本文复制引用

杨海燕,李孝攀,罗玉辉,杨海涛,木繁..耀变体PKS2155-304的光学波段光变特性[J].云南师范大学学报(自然科学版),2017,37(6):1-5,5.

基金项目

云南省教育厅科学研究基金资助性项目(2016ZZX230,2017ZZX079). (2016ZZX230,2017ZZX079)

云南师范大学学报(自然科学版)

OACSTPCD

1007-9793

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