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

Physics – Optics

Scientific paper

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Black Hole Physics, Galaxies: Individual (Ngc 1265), Galaxies: Elliptical And Lenticular, Cd, Galaxies: Kinematics And Dynamics, Instrumentation: Adaptive Optics

Scientific paper

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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