• DOI:10.1086/519301
• Corpus ID: 14027663

HD 98800: A 10 Myr Old Transition Disk

@article{Furlan2007HD9A,
  title={HD 98800: A 10 Myr Old Transition Disk},
  author={Elise Furlan and Benjamin A. Sargent and Nuria Calvet and William J. Forrest and Paola d’Alessio and Lee Hartmann and Dan M. Watson and Joel D. Green and Joan Rie Najita and C.-H. Chen},
  journal={The Astrophysical Journal},
  year={2007},
  volume={664},
  pages={1176 - 1184}
}

• E. Furlan, B. Sargent, +7 authors C.-H. Chen
• Published 2 May 2007
• Physics, Geology
• The Astrophysical Journal

We present the mid-infrared spectrum, obtained with the Spitzer Infrared Spectrograph (IRS), of HD 98800, a quadruple star system located in the 10 Myr old TW Hydrae association. It has a known mid-infrared excess that arises from a circumbinary disk around the B components of the system. The IRS spectrum confirms that the disk around HD 98800B displays no excess emission below about 5.5 μm, implying an optically thick disk wall at 5.9 AU and an inner, cleared-out region; however, some optically thin dust, consisting mainly of 3 μm-sized silicate dust grains, orbits the binary in a ring between 1.5 and 2 AU. The peculiar structure and apparent lack of gas in the HD 98800B disk suggests that this system is likely already at the debris disks stage, with a tidally truncated circumbinary disk of larger dust particles and an inner, second-generation dust ring, possibly held up by the resonances of a planet. The unusually large infrared excess can be explained by gravitational perturbations of the Aa+Ab pair puffing up the outer dust ring and causing frequent collisions among the larger particles.