A Resolved Ring of Debris Dust Around the Solar Analog HD 107146

S. A. Corder; J. M. Carpenter; A. I. Sargent; B. A. Zauderer; M. C. H. Wright; S. White; D. P. Woody; P. Teuben; S. L. Scott; M. W. Pound; R. L. Plambeck; J. W. Lamb; J. Koda; M. W. Hodges; D. W. Hawkins; D. C. -J. Bock

doi:10.1088/0004-637x/690/1/l65

arXiv · 0811.2713

A Resolved Ring of Debris Dust Around the Solar Analog HD 107146

S. A. Corder·J. M. Carpenter·A. I. Sargent·B. A. Zauderer·M. C. H. Wright·S. White·D. P. Woody·P. Teuben·S. L. Scott·M. W. Pound·R. L. Plambeck·J. W. Lamb·J. Koda·M. W. Hodges·D. W. Hawkins·D. C. -J. Bock

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Abstract

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 $λ$1.3 mm and the CSO at $λ$350 $μ$m. Both images show that the dust emission extends over an $\sim$10\arcsec diameter region. The high resolution (3\arcsec) CARMA image further reveals that the dust is distributed in a partial ring with significant decrease in flux inward of 97 AU. Two prominent emission peaks appear within the ring separated by $\sim$140 degrees in position angle. The morphology of the dust emission is suggestive of dust captured into a mean motion resonance, which would imply the presence of a planet at an orbital radius of $\sim$45-75 AU.

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S. A. Corder, J. M. Carpenter, A. I. Sargent, B. A. Zauderer, M. C. H. Wright, S. White, D. P. Woody, P. Teuben, S. L. Scott, M. W. Pound, R. L. Plambeck, J. W. Lamb, J. Koda, M. W. Hodges, D. W. Hawkins, D. C. -J. Bock. 2008-12-09. A Resolved Ring of Debris Dust Around the Solar Analog HD 107146. https://doi.org/10.1088/0004-637x/690/1/l65

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