An Edge-on Circumstellar Disk in the Young Binary System HK Tauri
Open accessAbstract
Hubble Space Telescope ( HST ) images of HK Tauri reveal that the companion star in this 2 4 (340 AU) pre-main-sequence binary system is an entirely nebulous object at visual wavelengths. HK Tau/c appears as two elongated reflection nebulosities separated by a dark lane. Near-infrared adaptive optics observations made at the Canada-France-Hawaii Telescope show a similar morphology and no directly visible star at λ≤2.2 μm. HK Tau/c is strikingly similar to scattered light models of an optically thick circumstellar disk seen close to edge-on and to the HST images of HH 30. HK Tau/c is therefore the first disk to be clearly resolved around an individual star in a young binary system. The disk properties have been constrained by fitting model reflection nebulae to the HST images. The disk has a radius of 105 AU, an inclination of about 5°, a scale height of 3.8 AU at r =50 AU, and is flared. The absence of a point source in the near-IR requires A V >50 mag toward the unseen central star. The thickness of the dark lane establishes a disk mass near 10 -4 M ☉ (~0.1 M Jupiter ) of dust and gas, if the dust grains have interstellar properties and remain fully mixed vertically. With the observed disk radius equal to one-third of the projected separation of the binary, there is a strong possibility that tidal truncation of the circumsecondary disk has occurred in this system.
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Disks have been imaged in wide binary T Tauri stars that are misaligned with the binary orbital plane.
“Disks have been imaged in wide binary T Tauri stars that are misaligned with the binary orbital plane (e.g., HK Tau; Stapelfeldt et al. 1998).”
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 Stapelfeldt et al. 1998
The Abstract reports an imaged circumstellar disk in HK Tau, a binary with a projected separation of 340 AU. Section 5.1 says the binary orbit is unlikely to be coplanar with the disk, but also says the orbital elements are unknown. The claim presents misalignment as established rather than inferred. (LLM, conf=0.88)
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- Authors
- Stapelfeldt, K. R., Krist, J. E., Ménard, F., Bouvier, J., Padgett, D. L., & Burrows, C. J.
- Affiliations
- Jet Propulsion Laboratory (US)
- Space Telescope Science Institute (US)
- Université Joseph Fourier (FR)
- California Institute of Technology (US)
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1998-07-20
- Volume
- 502
- Issue
- 1
- Pages
- L65-L69
- ISSN
- 0004-637X (ISSN-L)
- OpenAlex
- W2083293100
- Semantic Scholar
- 7ebc672e50c8565155fe3c3c0ad413d56e1060ce
- Cited by
- 252
- References
- 23
- Citations by year
- 2026: 3 · 2025: 5 · 2024: 1 · 2023: 1 · 2022: 4 · 2021: 4 · 2020: 10 · 2019: 3 · 2018: 6 · 2017: 5 · 2016: 8 · 2015: 4 · 2014: 8 · 2013: 10 · 2012: 10
- FWCI
- 15.21
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- 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 › Astro and Planetary Science
- Keywords
- circumstellar disks, edge-on disk, young binary stars, pre-main-sequence stars, reflection nebulae, scattered light, disk inclination, disk mass, tidal truncation, dark lanes, HH 30, disk flaring
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