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Detection of Intrinsic Source Structure at ∼3 Schwarzschild Radii with Millimeter-VLBI Observations of SAGITTARIUS A*

Ru-Sen Lu,Thomas P. Krichbaum,Alan L. Roy,Vincent L. Fish,Sheperd S. Doeleman,Michael D. Johnson,Kazunori Akiyama,Dimitrios Psaltis,Walter Alef,Keiichi Asada,Christopher Beaudoin,Alessandra Bertarini,Lindy Blackburn,Ray Blundell,Geoffrey C. Bower,Christiaan Brinkerink,Avery E. Broderick,Roger Cappallo,Geoffrey B. Crew,Jason Dexter,Matt Dexter,Heino Falcke,Robert Freund,Per Friberg,Christopher H. Greer,Mark A. Gurwell,Paul T. P. Ho,Mareki Honma,Makoto Inoue,Junhan Kim,James Lamb,Michael Lindqvist,David Macmahon,Daniel P. Marrone,Ivan Marti-Vidal,Karl M. Menten,James M. Moran,Neil M. Nagar,Richard L. Plambeck,Rurik A. Primiani,Alan E. E. Rogers,Eduardo Ros,Helge Rottmann,Jason SooHoo,Justin Spilker,Jordan Stone,Peter Strittmatter,Remo P. J. Tilanus,Michael Titus,Laura Vertatschitsch,Jan Wagner,Jonathan Weintroub,Melvyn Wright,Ken H. Young,J. Anton Zensus,Lucy M. Ziurys

The Astrophysical Journal（2018）

Cited 100|Views105
Key words
Galaxy: center,submillimeter: general,techniques: high angular resolution,techniques: interferometric
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