Correlated radio and optical variability in the BL Lacertae object 0716 + 714

Details Correlated radio and optical variability in the BL Lacertae object 0716 + 714 Correlated radio and optical variability in the BL Lacertae object 0716 + 714

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...372l..71q&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 372, May 10, 1991, p. L71-L74. DFG-supported research.

Astronomy and Astrophysics

Astronomy

149

Bl Lacertae Objects, Quasars, Radio Astronomy, Radio Jets (Astronomy), Radio Sources (Astronomy), Data Reduction, Light Curve, Very Large Array (Vla)

Scientific paper

Results are presented from simultaneous optical and radio observations of the BL Lacertae object 0716 + 714. During a 4-week period of continuous monitoring the source displayed in both wavelength regimes a transition between states of fast and slow variability with a change of the typical variability time scale from about 1 day to about 7 days. The simultaneous transition is interpreted as evidence for intrinsic source variability, and some consequences for the optical and radio emission regions are discussed.

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