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The circumbinary disk of HD 98800B: Evidence for disk warping

Akeson, R. L. and Rice, W. K. M. and Boden, A. F. and Sargent, A. I. and Carpenter, J. M. and Bryden, G. (2007) The circumbinary disk of HD 98800B: Evidence for disk warping. Astrophysical Journal, 670 (2). pp. 1240-1246. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:AKEapj07

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Abstract

The quadruple young stellar system HD 98800 consists of two spectroscopic binary pairs with a circumbinary disk around the B component. Recent work by Boden and collaborators using infrared interferometry and radial velocity data resulted in a determination of the physical orbit for HD 98800B. We use the resulting inclination of the binary and the measured extinction toward the B component stars to constrain the distribution of circumbinary material. Although a standard optically and geometrically thick disk model can reproduce the spectral energy distribution, it cannot account for the observed extinction if the binary and the disk are coplanar. We next constructed a dynamical model to investigate the influence of the A component, which is not in the Ba‐Bb orbital plane, on the B disk. We find that these interactions have a substantial impact on the inclination of the B circumbinary disk with respect to the Ba‐Bb orbital plane. The resulting warp would be sufficient to place material into the line of sight and the noncoplanar disk orientation may also cause the upper layers of the disk to intersect the line of sight if the disk is geometrically thick. These simulations also support that the dynamics of the Ba‐Bb orbit clear the inner region to a radius of~3 AU. We then discuss whether the somewhat unusual properties of the HD 98800B disk are consistent with material remnant from the star formation process or with more recent creation by collisions from larger bodies.


Item Type:Article
ORCID:
AuthorORCID
Akeson, R. L.0000-0001-9674-1564
Sargent, A. I.0000-0002-4633-5098
Additional Information:© 2007. The American Astronomical Society. Received 2007 May 21; accepted 2007 August 16. We thank Sverre Aarseth for help with the use of his N‐body codes and Kenneth Wood for initial SED modeling. We also thank Peter Brand and Mark Wyatt for useful discussions about secular perturbation theory. We are grateful to the anonymous referee for several helpful suggestions.
Group:Infrared Processing and Analysis Center (IPAC)
Subject Keywords:binaries: spectroscopic—circumstellar matter—stars: formation—stars: individual (HD 98800B)
Issue or Number:2
Record Number:CaltechAUTHORS:AKEapj07
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:AKEapj07
Alternative URL:http://dx.doi.org/10.1086/522579
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:9568
Collection:CaltechAUTHORS
Deposited By: Lindsay Cleary
Deposited On:05 Feb 2008
Last Modified:17 May 2017 16:39

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