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NASA NTRS · 20070021668

Observing NGC 4151 with the Keck Interferometer

Abstract

Observations of the nucleus of NGC 4151 at 2.2 microns using the two 10-meter Keck telescopes as an interferometer show a marginally resolved source less than or equal to 0.1 pc in diameter. These observations are the first measurement of an extragalactic source with an optical/IR interferometer. These observations represent a ten-fold improvement in angular resolution when compared to previous near-infrared measurements of AGN and make it possible to test the subparsecscale, near-infrared emission models of NGC 4151.

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BibTeXRIS

Swain, Mark R.. 2004-06-21. Observing NGC 4151 with the Keck Interferometer. https://ntrs.nasa.gov/citations/20070021668

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