Research Article
Signature of Plausible Accreting Supermassive Black Holes in Mrk 261/262 and Mrk 266
Table 1
The characteristics of the [OIII](λ 5007) km/s line from nuclear spectra in Mrk 261/262 and Mrk 266. Columns: (1) name; (2) redshift; (3) FWHM of the line [OIII]λ5007 in km/s; and (4) is the width of the [OIII]λ5007 line as a proxy for the stellar velocity dispersion on logarithmic scale.
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