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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S267(5), p. 195-195, 2009

DOI: 10.1017/s1743921310006150

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Searching for the Supermassive Black Hole in NGC 1265 (3C 83.1B)

Journal article published in 2009 by Alessandra Beifiori, Marc Sarzi, Roger L. Davies, Michele Cappellari, Ryan C. W. Houghton
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

We present K-band adaptive-optics assisted spectroscopic observations of the central region of the archetype head-tail radio galaxy NGC 1265 (3C 83.1), with the aim of constraining the mass of the supermassive black hole (MBH). The near-infrared data taken with the Altair–NIRI system on the Gemini North have a spatial resolution of FWHM = 0.”11 (39 pc, at the galaxy's distance of 73 Mpc).

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