The DOI matches its Crossref record; 23 of the 23 references it cites were found in a registry or an index.
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.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
The source backs part of the claim, not all of it — or backs it for a different population, condition or comparison.
In the citing paper
“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
Experimental — accuracy not yet measured
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Dynamics of binary-disk interaction. 1: Resonances and disk gap sizes
Artymowicz, P., & Lubow, S. H. (1994) · The Astrophysical Journal · doi:10.1086/173679 · Cited by 1,317
A Survey for Circumstellar Disks around Young Stellar Objects
Beckwith, S., Sargent, A., Chini, R., & Guesten, R. (1990) · The Astronomical Journal · doi:10.1086/115385 · Cited by 1,270
The Photometric Performance and Calibration of WFPC2
Holtzman, J. A., Burrows, C. J., Casertano, S., Hester, J. J., Trauger, J. T., Watson, A. M., & Worthey, G. (1995) · Publications of the Astronomical Society of the Pacific · doi:10.1086/133664 · Cited by 1,069
Self-citationDisk Accretion and Mass Loss from Young Stars
Hartigan, P. M., Edwards, S., & Ghandour, L. (1995) · The Astrophysical Journal · doi:10.1086/176344 · Cited by 973
Observational studies of pre-main-sequence evolution
Cohen, M., & Kuhi, L. V. (1979) · The Astrophysical Journal Supplement Series · doi:10.1086/190641 · Cited by 803
Strom, K. M., Strom, S. E., Edwards, S., Cabrit, S., & Skrutskie, M. F. (1989) · The Astronomical Journal · doi:10.1086/115085 · Cited by 783
D'Antona, F. A., & Mazzitelli, I. (1994) · The Astrophysical Journal Supplement Series · doi:10.1086/191867 · Cited by 672
Particle emissivity in circumstellar disks
Beckwith, S. V. W., & Sargent, A. I. (1991) · The Astrophysical Journal · doi:10.1086/170646 · Cited by 489
Hubble Space Telescope Observations of the Disk and Jet of HH 30
Burrows, C. J., Stapelfeldt, K. R., Watson, A. M., Krist, J., Ballester, G. E., Clarke, J. T., Crisp, D., Gallagher, J. S., Griffiths, R. E., Hester, J. J., et al. (1996) · The Astrophysical Journal · doi:10.1086/178156 · Cited by 434
Self-citationA new optical extinction law and distance estimate for the Taurus-Auriga molecular cloud
Kenyon, S. J., Dobrzycka, D., & Hartmann, L. W. (1994) · The Astronomical Journal · doi:10.1086/117200 · Cited by 340
Research works printed but not linked: 5
- Casali M. M., 1992, JCMT-UKIRT Newsl., 3, 33
- Moneti A., 1991, A&A, 242, 428
- Padgett D. L., 1997, BAAS, 29, 1360
- Shu, F., Najita, J., Galli, D., Ostriker, E. & Lizano, S. 1993, in Protostars and Planets III, ed. E. H. Levy & J. I. Lunine (Tuscon: Univ. Arizona Press), 3
- Whitney B. A., 1995, Rev. Mexicana Astron. Astrofis. Serie de Conferencias, 1, 201
Cited by
Sorted by citations
The James Webb Space Telescope
Gardner, J. P., Mather, J. C., Clampin, M., Doyon, R., Greenhouse, M., Hammel, H. B., Hutchings, J. B., Jakobsen, P., Lilly, S., Long, K. S., et al. (2006) · Space Science Reviews · doi:10.1007/s11214-006-8315-7 · Cited by 629
Protoplanetary Disks and Their Evolution
Williams, J. P., & Cieza, L. A. (2011) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081710-102548 · Cited by 1,403
Robitaille, T., Whitney, B. A., Indebetouw, R., & Wood, K. (2007) · The Astrophysical Journal Supplement Series · doi:10.1086/512039 · Cited by 870
The formation of a star cluster: predicting the properties of stars and brown dwarfs
Bate, M., Bonnell, I., & Bromm, V. (2002) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06210.x · Cited by 607
High-Energy Processes in Young Stellar Objects
Feigelson, E. D., & Montmerle, T. (1999) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.37.1.363 · Cited by 729
Metadata
- 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 › Earth and Planetary Sciences › Space and Planetary Science › 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
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review