GAMMA-RAY AND OPTICAL OSCILLATIONS IN PKS 0537-441

被引:40
|
作者
Sandrinelli, A. [1 ,2 ]
Covino, S. [2 ]
Treves, A. [1 ,2 ,3 ]
机构
[1] Univ Insubria, Via Valleggio 11, I-22100 Como, Italy
[2] INAF Inst Nazl Astrofis, Osservatorio Astron Brera, Via Emilio Bianchi 46, I-23807 Merate, Italy
[3] Ist Nazl Fis Nucl, Sez Trieste, Via Valerio 2, I-34127 Trieste, Italy
来源
ASTROPHYSICAL JOURNAL | 2016年 / 820卷 / 01期
关键词
BL Lacertae objects: general; BL Lacertae objects: individual (PKS 0537-441); galaxies: jets; gamma rays: galaxies; gamma rays: general; QUASI-PERIODIC OSCILLATION; TIME-SERIES; OJ; 287; BLAZARS; VARIABILITY; OBJECT; TELESCOPE; OUTBURST; BINARY; REM;
D O I
10.3847/0004-637X/820/1/20
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have considered the Fermi gamma-ray light curve of the blazar PKS 0537-441 during a high state extending from 2008 August 10 to 2011 August 27. The periodogram exhibits a peak at T similar to 280 days, with a significance of similar to 99.7%. A peak of similar relevance at 1/2T is found in the optical light curves. Considering the entire duration of the Fermi light curve 2008-2015, no significant peak is revealed, while the optical one remains meaningful. Comparing with recent observations of PKS 2155-304 and PG 1553+113 it seems that month-year oscillations can characterize some blazars. Month-scale oscillations can also show up only during phases of enhanced or bursting emission, such as in the case of PKS 0537-441.
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页数:6
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