Abstract
We present new spectroscopic identifications of 12 X-shaped radio galaxies and use the spectral data to derive starburst histories and masses of the nuclear supermassive black holes in these galaxies. The observations were done with the 2.1-m telescope of the Observatorio Astronómico Nacional at San Pedro Mártir, México. The new spectroscopic results extend the sample of X-shaped radio galaxies studied with optical spectroscopy. We show that the combined sample of the X-shaped radio galaxies has statistically higher black-hole masses and older episodes of star formation than a control sample of canonical double-lobed radio sources with similar redshifts and luminosities. The data reveal enhanced star-formation activity in the X-shaped sample on the timescales expected in galactic mergers. We discuss the results obtained in the framework of the merger scenario. © ESO, 2012.
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CITATION STYLE
Mezcua, M., Chavushyan, V. H., Lobanov, A. P., & León-Tavares, J. (2012). Starbursts and black hole masses in X-shaped radio galaxies: Signatures of a merger event? Astronomy and Astrophysics, 544. https://doi.org/10.1051/0004-6361/201117724
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