IUE observations of the BL Lac object AO 0235 + 164

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Spectroscopic monitoring of the BL Lac object AO 0235 + 164 ⋆

Aims. Spectroscopic monitoring of BL Lac objects is a difficult task that nonetheless can provide important information on the different components of the active galactic nucleus. Methods. We performed optical spectroscopic monitoring of the BL Lac object AO 0235+164 (z = 0.94) with the VLT and TNG telescopes from Aug. 2003 to Dec. 2004, during an extended WEBT campaign. The flux of this source...

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Unusual radio variability in the BL Lac object 0235 + 164

We present radio observations at three frequencies and contemporaneous optical monitoring of the peculiar BLLac object AO0235+164. During a three-week campaign with the VLA we observed intraday variability in this source and found a distinct peak which can be identified throughout the radio frequencies and tentatively connected to the R-band variations. This event is characterized by unusual pr...

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Harmonic QPOs and Thick Accretion Disk Oscillations in BL Lac Object AO 0235 + 164

Periodic outbursts are observed in many AGNs and usually explained with a supermassive black hole binary (SMBHB) scenario. However, multiple periods are observed in some AGNs and cannot be explained with it. Here we analyze the periodicity of the radio light curves of AO 0235+164 at multi-frequencies and report the discovery of six QPOs in integer ratio 1:2:3:4:5:6 of QPO frequencies, of which ...

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Unusual radio variability in the BL Lacertae object 0235 + 164

We present radio observations at three frequencies and contemporaneous optical monitoring of the peculiar BL Lac object AO 0235+164. During a three-week campaign with the VLA we observed intraday variability in this source and found a distinct peak which can be identified throughout the radio frequencies and tentatively connected to the R-band variations. This event is characterized by unusual ...

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 1982

ISSN: 0035-8711,1365-2966

DOI: 10.1093/mnras/201.3.801