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A Resolved Ring of Debris Dust Around the Solar Analog HD 107146
S. A. Corder, J. M. Carpenter, A. I. Sargent +13
We present resolved images of the dust continuum emission from the debris disk around the young (80-200 Myr) solar-type star HD 107146 with CARMA at 1.3 mm and the CSO at 350…
Event-horizon-scale structure in the supermassive black hole candidate at the Galactic Centre
Sheperd Doeleman, Jonathan Weintroub, Alan E. E. Rogers +25
The cores of most galaxies are thought to harbour supermassive black holes, which power galactic nuclei by converting the gravitational energy of accreting matter into radiation (r…
Molecular Gas in the z=1.2 Ultraluminous Merger GOODS J123634.53+621241.3
David T. Frayer, Jin Koda, Alexandra Pope +14
We report the detection of CO(2-1) emission from the z=1.2 ultraluminous infrared galaxy (ULIRG) GOODS J123634.53+621241.3 (also known as the sub-millimeter galaxy GN26). These obs…
Proplyds and Massive Disks in the Orion Nebula Cluster Imaged with CARMA and SMA
J. A. Eisner, R. L. Plambeck, John M. Carpenter +3
[Abridged] We imaged a 2' x 2' region of the Orion Nebula cluster in 1.3 mm wavelength continuum emission with the recently commissioned Combined Array for Research in Millimeter A…
A Parallactic Distance of 389 +24/-21 parsecs to the Orion Nebula Cluster from Very Long Baseline Array Observations
Karin M. Sandstrom, J. E. G. Peek, Geoffrey C. Bower +2
We determine the parallax and proper motion of the flaring, non-thermal radio star GMR A, a member of the Orion Nebula Cluster, using Very Long Baseline Array observations. Based o…
Giant Molecular Clouds in M33 - I. BIMA All Disk Survey
G. Engargiola, R. Plambeck, E. Rosolowsky +1
We present the first interferometric CO(J=1->0) map of the entire H-alpha disk of M33. The 13" diameter synthesized beam corresponds to a linear resolution of 50 pc, sufficient to…