TRUNCATED DISKS IN TW Hya ASSOCIATION MULTIPLE STAR SYSTEMS
Open accessAbstract
We present high angular resolution (down to 0 3 ≈ 13 AU in diameter) Submillimeter Array observations of the 880 μm (340 GHz) thermal continuum emission from circumstellar dust disks in the nearby HD 98800 and Hen 3-600 multiple star systems. In both cases, the dust emission is resolved and localized around one stellar component—the HD 98800B and Hen 3-600A spectroscopic binaries—with no evidence for circum-system material. Using two-dimensional Monte Carlo radiative transfer calculations, we compare the Submillimeter Array interferometer visibilities and broadband spectral energy distributions with truncated disk models to empirically locate the inner and outer edges of both disks. The HD 98800B disk appears to be aligned with the spectroscopic binary orbit, is internally truncated at a radius of 3.5 AU, and extends to only 10–15 AU from the central stars. The Hen 3-600A disk is slightly larger, with an inner edge at ∼1 AU and an outer radius of 15–25 AU. These inferred disk structures compare favorably with theoretical predictions of their truncation due to tidal interactions with the stellar companions.
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A disk in a binary system might extend all the way to its Roche radius with ξ about 1.
“A disk in a binary system might extend all the way to its Roche radius (Lin & Papaloizou 1993;Artymowicz & Lubow 1994;Andrews et al. 2010) with ξ ∼ 1.”
From PLANETARY CONSTRUCTION ZONES IN OCCULTATION: DISCOVERY OF AN EXTRASOLAR RING SYSTEM TRANSITING A YOUNG SUN-LIKE STAR AND FUTURE PROSPECTS FOR DETECTING ECLIPSES BY CIRCUMSECONDARY AND CIRCUMPLANETARY DISKS (2012) · cites this paper as Andrews et al. 2010
The Discussion reports that Hen 3-600A’s inferred outer disk edge of 15–25 AU agrees with a predicted tidal-truncation radius of about 25 AU. This supports the possibility of a disk reaching a binary-imposed outer limit, but our copy does not identify that limit as the Roche radius or give ξ ≈ 1. (LLM, conf=0.79)
Experimental — accuracy not yet measuredThe truncated disks of HD 98800 and Hen 3-600 are consistent with tidal truncation.
“The truncated disks of HD 98800 and Hen 3-600 are consistent with tidal truncation (Andrews et al. 2010).”
From PLANETARY CONSTRUCTION ZONES IN OCCULTATION: DISCOVERY OF AN EXTRASOLAR RING SYSTEM TRANSITING A YOUNG SUN-LIKE STAR AND FUTURE PROSPECTS FOR DETECTING ECLIPSES BY CIRCUMSECONDARY AND CIRCUMPLANETARY DISKS (2012) · cites this paper as Andrews et al. 2010
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Mamajek, E. E., Quillen, A. C., Pecaut, M. J., Moolekamp, F., Scott, E. L., Kenworthy, M. A., Cameron, A. C., & Parley, N. R. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/143/3/72 · Cited by 140 · see citing works
“The truncated disks of HD 98800 and Hen 3-600 are consistent with tidal truncation (Andrews et al. 2010).”
Background
- Authors
- Andrews, S. M., Czekala, I., Wilner, D. J., Espaillat, C., Dullemond, C. P., & Hughes, A. M.
- Affiliations
- Center for Astrophysics Harvard & Smithsonian (US)
- Max Planck Institute for Astronomy (DE)
- Corresponding author
- Andrews, Sean M.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2010-01-19
- Volume
- 710
- Issue
- 1
- Pages
- 462-469
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2021965181
- Semantic Scholar
- 6e653142bfa89612b23a24aa0755f77155936ed0
- Cited by
- 87
- References
- 67
- Citations by year
- 2026: 1 · 2025: 3 · 2024: 1 · 2023: 2 · 2022: 3 · 2021: 4 · 2019: 9 · 2018: 21 · 2017: 8 · 2016: 3 · 2015: 4 · 2014: 4 · 2013: 4 · 2012: 10
- FWCI
- 4.29
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation (0754568, 0901947, NAS 5-26555)
- U.S. Department of Defense
- Smithsonian Institution
- National Aeronautics and Space Administration (NNG05GI81G, NAS 526555, 526555)
- Space Telescope Science Institute (NAS5- 26555, 5-26555, 26555)
- Academia Sinica
- Smithsonian Astrophysical Observatory
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Keywords
- TW Hya association, HD 98800, multiple star systems, spectroscopic binaries, tidal truncation, submillimeter continuum emission, radiative transfer modeling
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