A polarization flare in OJ 287

Details A polarization flare in OJ 287 A polarization flare in OJ 287

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.211..497h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 211, Dec. 1, 1984, p. 497-506. Research supported by th

Astronomy and Astrophysics

Astronomy

59

Astronomical Spectroscopy, Bl Lacertae Objects, Plasma Jets, Polarization Characteristics, Astronomical Models, Infrared Spectra, Near Infrared Radiation, Radiant Flux Density, Ubv Spectra, Visible Spectrum

Scientific paper

Observations of the BL Lac object OJ 287 were made simultaneously at
infrared JHK wavelengths and in optical and near infrared wavelengths at
UBVRI in 1983 January. These observations, of total flux reaching a peak
and then decaying, and of complex polarization changes, are explained in
terms of a model of a jet emanating from an accretion disc.

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