Next Article in Journal / Special Issue
Using the Pairs of Lines Broadened by Collisions with Neutral and Charged Particles for Gas Temperature Determination of Argon Non-Thermal Plasmas at Atmospheric Pressure
Previous Article in Journal
THz/Infrared Double Resonance Two-Photon Spectroscopy of HD+ for Determination of Fundamental Constants
Previous Article in Special Issue
Stark-Zeeman Line Shape Modeling for Magnetic White Dwarf and Tokamak Edge Plasmas: Common Challenges
Article Menu

Export Article

Open AccessFeature PaperProject Report
Atoms 2017, 5(4), 39; doi:10.3390/atoms5040039

Photometric and Polarimetric Interpretation of Blazar AO 0235+164 Behaviour

Department of Astrophysics, Faculty of Mathematics and Mechanics, Saint Petersburg State University, Saint Petersburg 199034, Russia
Academic Editors: Milan S. Dimitrijević and Luka Č. Popović
Received: 7 September 2017 / Revised: 30 September 2017 / Accepted: 3 October 2017 / Published: 19 October 2017
(This article belongs to the Special Issue Spectral Line Shapes in Astrophysics and Related Topics)
View Full-Text   |   Download PDF [2901 KB, uploaded 19 October 2017]   |  

Abstract

Among the great number of controversial issues, the most topical one both for theoretical and observational astrophysics presently is a problem of active galactic nuclei investigation. To explain the behaviour of blazar AO 0235+164, which has been under observation at the LX200 telescope (SPbSU) since 2002, the method of analyzing developed by V.A. Hagen-Thorn and S.G. Marchenko was applied. It is based on the assumption that in the case of observational data lying on the straight line in the absolute Stokes parameters space { I , Q , U } (for polarimetry) and the fluxes space { F 1 , . . F n } (for photometry), relative Stokes parameters and relative flux ratios stay unchanged , and consequently, only one source is corresponding to the variability of general value of flux. In this paper, the photometric and polarimetric interpretation of blazar behaviour is presented. Furthermore, the flux and flux–flux diagrams are obtained for three periods of object monitoring: 2006–2007 and 2008–2009 (outbursts) and 2009–2016 (decline with 2015 outburst). View Full-Text
Keywords: active galaxies; BL Lacertae objects; AO 0235+164; photometry; polarimetry active galaxies; BL Lacertae objects; AO 0235+164; photometry; polarimetry
Figures

Figure 1

This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (CC BY 4.0).

Scifeed alert for new publications

Never miss any articles matching your research from any publisher
  • Get alerts for new papers matching your research
  • Find out the new papers from selected authors
  • Updated daily for 49'000+ journals and 6000+ publishers
  • Define your Scifeed now

SciFeed Share & Cite This Article

MDPI and ACS Style

Shablovinskaya, E. Photometric and Polarimetric Interpretation of Blazar AO 0235+164 Behaviour. Atoms 2017, 5, 39.

Show more citation formats Show less citations formats

Note that from the first issue of 2016, MDPI journals use article numbers instead of page numbers. See further details here.

Related Articles

Article Metrics

Article Access Statistics

1

Comments

[Return to top]
Atoms EISSN 2218-2004 Published by MDPI AG, Basel, Switzerland RSS E-Mail Table of Contents Alert
Back to Top