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A compact radio source in the nucleus of M87

Abstract

The nucleus and jet of the giant elliptical galaxy M87 have been studied at radio wavelengths with resolutions ranging upwards from a few milliarc seconds1–3. The higher-resolution maps show that the nucleus consists of a bright central region with a feature with smoothly decaying brightness pointing in the direction of the larger-scale radio/optical/X-ray jet. Moreover, these maps indicate that collimation of the jet occurs within 10 marc s of the nucleus (that is, within 1 pc of the nucleus, as M87 lies at a distance of 12–20 Mpc4). We report here high-resolution, very-long-baseline interferometric (VLBI) observations at 1.35 cm wavelength, which reveal the existence of a compact core (0.2 marc s) and an associated extended feature (0.3 marc s), again pointing in the same direction as the large-scale jet. Our observations show that the radio jet is formed on a size scale of 10−2pc, thus strengthening the evidence for the presence of a massive black hole in the nucleus of M87.

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Spencer, R., Junor, W. A compact radio source in the nucleus of M87. Nature 321, 753–755 (1986). https://doi.org/10.1038/321753a0

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