Krist, John E. and Stapelfeldt, Karl R. and Bryden, Geoffrey and Rieke, George H. and Su, K. Y. L. and Chen, Christine C. and Beichman, Charles A. and Hines, Dean C. and Rebull, Luisa M. and Tanner, Angelle and Trilling, David E. and Clampin, Mark and Gáspár, András (2010) HST and Spitzer Observations of the HD 207129 Debris Ring. Astronomical Journal, 140 (4). pp. 1051-1061. ISSN 0004-6256 http://resolver.caltech.edu/CaltechAUTHORS:20100929-111919827
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A debris ring around the star HD 207129 (G0V; d = 16.0 pc) has been imaged in scattered visible light with the ACS coronagraph on the Hubble Space Telescope (HST) and in thermal emission using MIPS on the Spitzer Space Telescope at λ = 70 μm (resolved) and 160 μm (unresolved). Spitzer IRS (λ = 7-35 μm) and MIPS (λ = 55-90 μm) spectrographs measured disk emission at λ> 28 μm. In the HST image the disk appears as a ~30 AU wide ring with a mean radius of ~163 AU and is inclined by 60° from pole-on. At 70 μm, it appears partially resolved and is elongated in the same direction and with nearly the same size as seen with HST in scattered light. At 0.6 μm, the ring shows no significant brightness asymmetry, implying little or no forward scattering by its constituent dust. With a mean surface brightness of V = 23.7 mag arcsec^(–2), it is the faintest disk imaged to date in scattered light. We model the ring's infrared spectral energy distribution (SED) using a dust population fixed at the location where HST detects the scattered light. The observed SED is well fit by this model, with no requirement for additional unseen debris zones. The firm constraint on the dust radial distance breaks the usual grain size-distance degeneracy that exists in modeling of spatially unresolved disks, and allows us to infer a minimum grain size of ~2.8 μm and a dust size distribution power-law spectral index of –3.9. An albedo of ~5% is inferred from the integrated brightness of the ring in scattered light. The low-albedo and isotropic scattering properties are inconsistent with Mie theory for astronomical silicates with the inferred grain size and show the need for further modeling using more complex grain shapes or compositions. Brightness limits are also presented for six other main-sequence stars with strong Spitzer excess around which HST detects no circumstellar nebulosity (HD 10472, HD 21997, HD 38206, HD 82943, HD 113556, and HD 138965).
|Additional Information:||© 2010 American Astronomical Society. Received 2010 April 26; accepted 2010 August 14; published 2010 September 9. We thank Paul Smith (University of Arizona) for his assistance with the MIPS SED data, and Karl Misselt and Viktor Zubko for calculating optical properties of grains at large size parameters. This work was supported by Hubble Space Telescope General Observer Grant 10539 to the Jet Propulsion Laboratory, California Institute of Technology and by the Spitzer Project Science Office at JPL. Funding from both was provided by the National Aeronautics and Space Administration. The Spitzer Space Telescope is operated by the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract 1407.|
|Subject Keywords:||circumstellar matter; stars: individual (HD 207129, HD 10472, HD 21997, HD 38206, HD 82943, HD 113556, HD 138965, HD 211415)|
|Classification Code:||PACS: 97.21.+a; 97.10.Fy; 95.85.Hp; 95.85.Mt; 98.58.Ca; 95.85.Kr|
|Official Citation:||John E. Krist et al 2010 The Astronomical Journal 140 1051 doi: 10.1088/0004-6256/140/4/1051|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Jason Perez|
|Deposited On:||29 Sep 2010 20:40|
|Last Modified:||26 Dec 2012 12:28|
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