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Observing NGC 4151 with the Keck interferometer

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dc.contributor.author Swain, Mark R.
dc.date.accessioned 2006-11-28T19:37:03Z
dc.date.available 2006-11-28T19:37:03Z
dc.date.issued 2004-06-21
dc.identifier.citation SPIE Astronomical Telescopes and Instrumentation, Glasgow, Scotland, June 21, 2004. en
dc.identifier.clearanceno 04-1540
dc.identifier.uri http://hdl.handle.net/2014/40008
dc.description.abstract Observations of the nucleus of NGC 41 5 1 at 2.2 pm 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 optica/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. en
dc.description.sponsorship NASA/JPL en
dc.format.extent 1404810 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US en
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2004. en
dc.subject interferometry en
dc.subject Active Galactic Nuclei (AGN) en
dc.title Observing NGC 4151 with the Keck interferometer en
dc.type Preprint en


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