Protoplanetary disk structures in Ophiuchus

Andrews, Sean M.; Wilner, D. J.; Hughes, A. M.; Qi, Chunhua; Dullemond, C. P.

doi:10.1088/0004-637x/700/2/1502

Cited by 709Astrophysics and Star Formation StudiesAstro and Planetary ScienceStellar, planetary, and galactic studies

Protoplanetary disk structures in Ophiuchus

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Andrews, Sean M., Wilner, D. J., Hughes, A. M., Qi, Chunhua, Dullemond, C. P.·2009·The Astrophysical Journal

DOI 10.1088/0004-637x/700/2/1502

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Abstract

We present the results of a high angular resolution (0 3 ≈ 40 AU) Submillimeter Array survey of the 345 GHz (870 μm) thermal continuum emission from nine of the brightest, and therefore most massive, circumstellar disks in the ∼1 Myr-old Ophiuchus star-forming region. Using two-dimensional radiative transfer calculations, we simultaneously fit the observed continuum visibilities and broadband spectral energy distribution for each disk with a parametric structure model. Compared to previous millimeter studies, this survey includes significant upgrades in modeling, data quality, and angular resolution that provide improved constraints on key structure parameters, particularly those that characterize the spatial distribution of mass in the disks. In the context of a surface density profile motivated by similarity solutions for viscous accretion disks, Σ ∝ ( R / R c ) −γ exp [ − ( R / R c ) 2−γ ], the best-fit models for the sample disks have characteristic radii R c ≈ 20–200 AU, high disk masses M d ≈ 0.005–0.14 M ☉ (a sample selection bias), and a narrow range of radial Σ gradients (γ ≈ 0.4–1.0) around a median γ = 0.9. These density structures are used in conjunction with accretion rate estimates from the literature to help characterize the viscous evolution of the disk material. Using the standard prescription for disk viscosities, those combined constraints indicate that α ≈ 0.0005–0.08. Three of the sample disks show large ( R ≈ 20–40 AU) central cavities in their continuum emission morphologies, marking extensive zones where dust has been physically removed and/or has significantly diminished opacities. Based on the current requirements of planet formation models, these emission cavities and the structure constraints for the sample as a whole suggest that these young disks may eventually produce planetary systems, and have perhaps already started.

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Gas and Dust Emission at the Outer Edge of Protoplanetary Disks
Hughes, A. M., Wilner, D. J., Qi, C., & Hogerheijde, M. R. (2008) · The Astrophysical Journal · doi:10.1086/586730 · Cited by 175 · see citing works
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Near-Infrared Spectra and the Evolutionary Status of Young Stellar Objects: Results of a 1.1-2.4 (??) Survey
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Optical Spectroscopy of the Surface Population of the ρ Ophiuchi Molecular Cloud: The First Wave of Star Formation
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Photoevaporation of protoplanetary discs I: hydrodynamic modelsPreprint
Alexander, R. D., Clarke, C. J., & Pringle, J. E. (2006) · Cited by 172 · see citing works
Resolving the inner dust disks surrounding LkCa 15 and MWC 480 at mm wavelengths
Piétu, V., Dutrey, A., Guilloteau, S., Chapillon, E., & Pety, J. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20065968 · Cited by 170 · see citing works
Sub-arcsec imaging of the AB Aur molecular disk and envelope at millimeter wavelengths: a non Keplerian disk
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Evolution of protoplanetary disks: Constraints from DM Tauri and GM Aurigae
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Fragmentation of Gravitationally Unstable Gaseous Protoplanetary Disks with Radiative Transfer
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Astrophysics of Young Star Binaries
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Dust filtration at gap edges: Implications for the spectral energy distributions of discs with embedded planetsPreprint
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Kuiper Belt Objects: Relics from the Accretion Disk of the Sun
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Evidence for Early Stellar Encounters in the Orbital Distribution of Edgeworth–Kuiper Belt Objects
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Hipparcos distance estimates of the Ophiuchus and the Lupus cloud complexes
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Large dust particles in disks around T Tauri stars
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AnIUEAtlas of Pre–Main‐Sequence Stars. II. Far‐Ultraviolet Accretion Diagnostics in T Tauri Stars
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The Formation and Habitability of Extra-Solar Planets
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An Inner Hole in the Disk around TW Hydrae Resolved in 7 mm Dust Emission
Hughes, A. M., Wilner, D. J., Calvet, N., D’Alessio, P., Claussen, M. J., & Hogerheijde, M. R. (2007) · The Astrophysical Journal · doi:10.1086/518885 · Cited by 155 · see citing works
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Formation of gas giant planets: core accretion models with fragmentation and planetary envelope
Inaba, S., Wetherill, G. W., & Ikoma, M. (2003) · Icarus · doi:10.1016/j.icarus.2003.08.001 · Cited by 154 · see citing works
VLA Imaging of the Disk Surrounding the Nearby Young Star TW Hydrae
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Demographics of Transition ObjectsPreprint
Najita, J. R., Strom, S. E., & Muzerolle, J. (2013) · Cited by 148 · see citing works
An unbiased search for the signatures of protostars in the ρ Ophiuchi molecular cloud
Stanke, T., Smith, M. D., Gredel, R., & Khanzadyan, T. (2006) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20041331 · Cited by 147 · see citing works
Millimeter imaging of HD 163296: probing the disk structure and kinematics
Isella, A., Testi, L., Natta, A., Neri, R., Wilner, D., & Qi, C. (2007) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20077385 · Cited by 141 · see citing works
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Gas Flow Across Gaps in Protoplanetary Disks 1Preprint
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Observations of T Tauri Disks at Sub‐AU Radii: Implications for Magnetospheric Accretion and Planet Formation
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Investigating Disk Evolution: A High Spatial Resolution Mid‐Infrared Survey of T Tauri Stars
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Imaging the HL Tauri Disk at λ = 2.7 Millimeters with the BIMA Array
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Terrestrial Planet Formation in Disks with Varying Surface Density Profiles
Raymond, S. N., Quinn, T., & Lunine, J. I. (2005) · The Astrophysical Journal · doi:10.1086/433179 · Cited by 119 · see citing works
Millimeter imaging of HD 163296: probing the disk structure and kinematics
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Pre-main sequence spectroscopic binaries suitable for VLTI observations
Guenther, E. W., Esposito, M., Mundt, R., Covino, E., Alcalá, J. M., Cusano, F., & Stecklum, B. (2007) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20065686 · Cited by 115 · see citing works
Resolving the Inner Dust Disks surrounding LkCa 15 and MWC 480 at mm wavelengths ⋆
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Confirmation of a Gapped Primordial Disk around LkCa 15
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Protostellar accretion disks resolved with the JCMT-CSO interferometer
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Constraints on the HL Tauri Protostellar Disk from Millimeter‐ and Submillimeter‐Wave Interferometry
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LkHα 330: Evidence for Dust Clearing through Resolved Submillimeter Imaging
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Secular evolution of viscous and self-gravitating circumstellar discs
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A catalog of co-added IRAS fluxes of Orion population stars
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Imaging the Small-Scale Circumstellar Gas Around T Tauri Stars
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Constraints on Properties of the Protoplanetary Disks around UX Orionis and CQ Tauri
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RAPID FORMATION OF ICY SUPER-EARTHS AND THE CORES OF GAS GIANT PLANETS
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An investigation of grain properties in the Rho Ophiuchi dark cloud
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Constraints on Circumstellar Disk Parameters from Multiwavelength Observations: T Tauri and SU Aurigae
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The submillimetre colour of young stellar objects
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MINIMUM MASS SOLAR NEBULAE AND PLANETARY MIGRATION
Crida, A. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/698/1/606 · Cited by 83 · see citing works
Observations of T Tauri Disks at Sub-AU Radii: Implications for Magnetospheric Accretion and Planet FormationPreprint
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A Keplerian disk around the Herbig Ae star HD 34282
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The effects of nebula surface density profile and giant‐planet eccentricities on planetary accretion in the inner solar system
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Planets Rapidly Create Holes in Young Circumstellar Disks
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The BP Tau disk: A missing link between Class II and III objects?
Dutrey, A., Guilloteau, S., & Simon, M. (2003) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20030317 · Cited by 70 · see citing works
Self-regulated gravitational accretion in protostellar discs
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A Minimum‐Mass Extrasolar Nebula
Kuchner, M. J. (2004) · The Astrophysical Journal · doi:10.1086/422577 · Cited by 64 · see citing works
Growth and Migration of Solids in Evolving Protostellar Disks. I. Methods and Analytical Tests
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From discs to planetesimals: Evolution of gas and dust discs
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The Surface Density Distribution in the Solar Nebula
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Analysis of the dust evolution in the circumstellar disks of T Tauri stars
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Resolving the circumbinary dust disk surrounding HH 30
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Emission-line studies of young stars. III - Correlations with the infrared excess
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Secular evolution of viscous and self-gravitating circumstellar discsPreprint
Vorobyov, E. I., & Basu, S. (2008) · Cited by 47 · see citing works
A Minimum Mass Extrasolar NebulaPreprint
Kuchner, M. J. (2003) · Cited by 45 · see citing works
Multiwavelength studies of the gas and dust disc of IRAS 04158+2805
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Mid-Infrared Imaging of Young Stellar Objects
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DISK MASSES IN THE EMBEDDED AND T TAURI PHASES OF STELLAR EVOLUTION
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Resolving and Probing the Circumstellar Disk of the Herbig Ae Star MWC 480 at λ = 1.4 mm: Evolved Dust?
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The Evolution of Circumstellar Disks in Ophiuchus Binaries
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The Structure of the DoAr 25 Circumstellar Disk
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THE EVOLUTION OF CIRCUMSTELLAR DISKS IN OPHIUCHUS BINARIES
Patience, J., Akeson, R., Jensen, E. L. N., Patience, J., Akeson, R. L., & Jensen, E. L. N. (2004) · Cited by 16 · see citing works
Physics and Astrophysics of Planetary Systems
Montmerle, T., Ehrenreich, D., & Lagrange, A. ‐. (2010) · Cited by 13 · see citing works

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Mind Your Ps and Qs: The Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars
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The Disk Substructures at High Angular Resolution Project (DSHARP). I. Motivation, Sample, Calibration, and Overview
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Authors: Andrews, S. M., Wilner, D. J., Hughes, A. M., Qi, C., & Dullemond, C. P.
Affiliations: Center for Astrophysics Harvard & Smithsonian (US)
Max Planck Institute for Astronomy (DE)
ORCID: Andrews, Sean M.
Wilner, D. J.
Hughes, A. M.
Qi, Chunhua
Dullemond, C. P.
Venue: The Astrophysical Journal
Publisher: American Astronomical Society
Published: 2009-07-14
Volume: 700
Issue: 2
Pages: 1502-1523
ISSN: 0004-637X (ISSN-L)
1538-4357
DOI: 10.1088/0004-637x/700/2/1502
OpenAlex: W2047712469
Cited by: 709
References: 168
Citations by year: 2026: 16 · 2025: 22 · 2024: 21 · 2023: 21 · 2022: 25 · 2021: 30 · 2020: 43 · 2019: 45 · 2018: 90 · 2017: 59 · 2016: 71 · 2015: 48 · 2014: 37 · 2013: 56 · 2012: 40
FWCI: 21.00
Type: journal article
Language: en
Open access: bronze
doi.org
Locations: The Astrophysical Journal (publishedVersion)
arXiv (Cornell University) (submittedVersion)
Max Planck Institute for Plasma Physics (submittedVersion)
arXiv (Cornell University)
Funders: National Aeronautics and Space Administration (NNG05GI81G, NAS 526555, 526555)
Space Telescope Science Institute (NAS5- 26555, 5-26555, 26555)
Topics: Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords: protoplanetary disks, Ophiuchus star-forming region, disk structure, surface density profile, disk mass, disk viscosity, accretion rate, disk cavity, dust removal, planet formation, radiative transfer modeling

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Protoplanetary disk structures in Ophiuchus

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