Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005mnras.360..119d&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 360, Issue 1, pp. 119-124.
Astronomy and Astrophysics
Astronomy
3
Galaxies: Active, Galaxies: Individual: Ngc 266, Galaxies: Seyfert, Radio Continuum: Galaxies, Submillimetre
Scientific paper
We report multi-frequency and multi-epoch radio continuum observations with multi-spatial resolution for the low-luminosity active galactic nucleus (LLAGN) NGC 266. In the centimetre regime, we find diffuse components with Very Large Array (VLA) observations, and a variable compact core with a rising spectrum with Very Long Baseline Array (VLBA) observations. Although the spectral index of the rising spectrum is consistent with the prediction of the simple advection-dominated accretion flow (ADAF) model, the observed radio power is slightly high compared with that of the model prediction. A spectral break at centimetre-to-millimetre wavelengths is inferred from the upper limits of flux densities from Nobeyama Millimetre Array (NMA) and James Clerk Maxwell Telescope (JCMT) data at millimetre and submillimetre wavelengths, respectively. More complicated considerations are required for the theoretical model to interpret such observed radio properties.
Doi Akihiro
Inoue Makoto
Kameno Seiji
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