Optical polarization angle and VLBI jet direction in the binary black hole model of OJ287
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/421/3/1861/5834447/mnras0421-1861.pdf
Reference47 articles.
1. LOCATION OF γ-RAY FLARE EMISSION IN THE JET OF THE BL LACERTAE OBJECT OJ287 MORE THAN 14 pc FROM THE CENTRAL ENGINE
2. VLBA Observations of Radio Reference Frame Sources. II. Astrometric Suitability Based on Observed Structure
3. VLBA Observations of Radio Reference Frame Sources. I.
4. The parsec-scale polarization structure of nine BL Lacertae objects at = 3.6 cm
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1. Evidence of Jet Activity from the Secondary Black Hole in the OJ 287 Binary System;The Astrophysical Journal Letters;2024-06-01
2. Quasi-simultaneous Optical Flux and Polarization Variability of the Binary Super Massive Black Hole Blazar OJ 287 from 2015 to 2023: Detection of an Anticorrelation in Flux and Polarization Variability;The Astrophysical Journal Letters;2023-10-30
3. Observational Implications of OJ 287’s Predicted 2022 Disk Impact in the Black Hole Binary Model;Galaxies;2023-07-03
4. X-Ray Studies of Blazar 1ES 1959+650 Using Swift and XMM-Newton Satellite;The Astrophysical Journal;2023-07-01
5. Correlation Analysis between OJ 287 Radio Jet Observables;The Astrophysical Journal;2023-05-01
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