A 34.5 day quasi-periodic oscillation in γ-ray emission from the blazar PKS 2247–131
PKS 2247–131 is an active galaxy that has been emitting gamma-ray flares since October 2016. Here, the authors used data obtained with the Fermi Gamma-ray Space Telescope to find that PKS 2247–131 presents a relatively short, month-like flux oscillation at gamma-ray energies of 0.1–300 GeV.
Saved in:
Main Authors: | Jianeng Zhou, Zhongxiang Wang, Liang Chen, Paul J. Wiita, Jithesh Vadakkumthani, Nidia Morrell, Pengfei Zhang, Jujia Zhang |
---|---|
Format: | article |
Language: | EN |
Published: |
Nature Portfolio
2018
|
Subjects: | |
Online Access: | https://doaj.org/article/be4286c0ba6f427ca63dc38ab71a1fbc |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Evolving parsec-scale radio structure in the most distant blazar known
by: Tao An, et al.
Published: (2020) -
Herpes Simplex Virus γ34.5 Interferes with Autophagosome Maturation and Antigen Presentation in Dendritic Cells
by: Philipe A. M. Gobeil, et al.
Published: (2012) -
Reprogramming of the antimycin NRPS-PKS assembly lines inspired by gene evolution
by: Takayoshi Awakawa, et al.
Published: (2018) -
Acta Nº345
by: Banco Central de Chile
Published: (2019) -
Acta No. 131
by: Banco Central de Chile
Published: (2019)