FINE-SCALE STRUCTURE OF THE QUASAR 3C 279 MEASURED WITH 1.3 mm VERY LONG BASELINE INTERFEROMETRY

We report results from five day very long baseline interferometry observations of the well-known quasar 3C 279 at 1.3 mm (230 GHz) in 2011. The measured nonzero closure phases on triangles including stations in Arizona, California, and Hawaii indicate that the source structure is spatially resolved....

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Bibliographic Details
Main Authors: Lu, Rusen (Contributor), Fish, Vincent L. (Contributor), Doeleman, Sheperd Samuel (Contributor), Crew, Geoffrey B. (Contributor), Cappallo, Roger J. (Contributor), Titus, Michael A. (Contributor)
Other Authors: Haystack Observatory (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-02-17T13:46:59Z.
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