Skip to main content
SpringerLink
Log in
Book cover

From Dust to Terrestrial Planets pp 55–68Cite as

Observational Constraints on Transport (And Mixing) in Pre-Main Sequence Disks

  • Conference paper

Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 9))

Abstract

Currently available observational constraints on transport mechanisms in pre-main sequence disks are reviewed. The main observable quantity accessable by imaging the spatial structure of disks is the mass accretion rate, which constrains angular momentum transport, and migration and diffusion of disk material.

This is a preview of subscription content, log in via an institution.

Chapter
USD   29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD   169.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD   219.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD   219.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Learn about institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  • Baibus, S.A., and Hawley, J.F.: 2000, ‘Solar Nebula Magnetohydrodynamics’, Space Sci. Rev. 92, this volume.

    Google Scholar 

  • Beckwith, S.V.W., and Sargent, A.I.: 1991, ‘Particle Emissivity in Circumstellar Disks’, Astrophys. J. 381, 250–258.

    Article  ADS  Google Scholar 

  • Beckwith, S.V.W., Sargent, A.I., Chini, R.S., and Güsten, R.: 1990, ‘A Survey for Circumstellar Disks Around Young Stellar Objects’, Astron. J. 99, 924–945

    Article  ADS  Google Scholar 

  • Bell, K.R., and Lin, D.N.C.: 1994, ‘Using FU Orionis Outbursts to Constrain Self-regulated Protostellar Disk Models’, Astrophys. J. 427, 987–1004.

    Article  ADS  Google Scholar 

  • Brandenburg, A., Nordlund, A., Stein, R. F., and Torkelsson, U.: 1996, ‘The Disk Accretion Rate for Dynamo-generated Turbulence’, Astrophys. J. 458, L45–L49.

    Article  ADS  Google Scholar 

  • Burrows, C.J., Stapelfeldt, K.R., Watson, A.M., Krist, J.E., Ballester, G.E., Clarke, J.T., Crisp, D., Gallagher III, J. S., Griffiths, R. E., Hester, J. J., Hoessel, J. G., Holtzman, J. A., Mould, J. R., Scowen, P.A., Trauger, J.T., and Westphal, J.A.: 1996, ‘Hubble Space Telescope Observations of the Disk and Jet of HH 30’, Astrophys. J. 473, 437–451.

    Article  ADS  Google Scholar 

  • Calvet, N.: 1997, ‘Disk Accretion in Pre-Main Sequence Stars’, in S.S. Holt and T. R. Kallman (eds.), Accretion Processes in Astrophysical Systems: Some Like it Hot!, AIP Conf. Proc. 431, 495–505.

    Google Scholar 

  • Calvet, N., and Gullbring, E.: 1998, ‘The Structure and Emission of the Accretion Shock in T Tauri Stars’, Astrophys. J. 509, 802–818.

    Article  ADS  Google Scholar 

  • Calvet, N., Hartmann, L., and Strom, S.E.: 2000, in V. Mannings, S. Russell, and A.P. Boss (eds.), Evolution of Disk Accretion, Protostars and Planets IV, Univ. of Arizona Press, Tucson, in press.

    Google Scholar 

  • Cassen, P.: 1994, ‘Utilitarian Models of the Solar Nebula’, Icarus 112, 405–429.

    Article  ADS  Google Scholar 

  • D’Alessio, P., Calvet, N., Hartmann, L., Canto, J., and Lizano, S.: 1999, ‘Accretion Disks around Young Objects. II. Well-Mixed Models with ISM Dust’, Astrophys. J., submitted.

    Google Scholar 

  • Drouart, A., Dubrulle, B., Gautier, D., and Robert, F.: 1999, ‘Structure and Transport in the Solar Nebula from Constraints on Deuterium Enrichment and Giant Planet Formation’, Icarus 140, 129–155.

    Article  ADS  Google Scholar 

  • Dutrey, A., Guilloteau, S., Duvert, G., Prato, L., Simon, M., Schuster, K., Menard, F.: 1996, ‘Dust and Gas Distribution Around T Tauri Stars in Taurus-Auriga. I. Interferometric 2.7mm Continuum and 13CO J=1−0 Observations’, Astron. Astrophys. 309, 493–504.

    ADS  Google Scholar 

  • Edwards, S., Hartigan, P., Ghandour, L., and Andrulis, C.: 1994, ‘Spectroscopic Evidence for Magnetospheric Accretion in Classical T Tauri stars’, Astron. J. 108, 1056–1070.

    Article  ADS  Google Scholar 

  • Gammie, C.: 1996, ‘Layered Accretion in T Tauri Disks’, Astrophys. J. 457, 355–362.

    Article  ADS  Google Scholar 

  • Gullbring, E., Hartmann, L., Briceno, C., and Calvet, N.: 1998, ‘Disk Accretion Rates for T Tauri Start’, Astrophys. J. 492, 323–341.

    Article  ADS  Google Scholar 

  • Hartigan, P., Strom, S.E., Edwards, S., Kenyon, S.J., Hartmann, L., Stauffer, J., and Welty, A.D.: 1991, ‘Optical Excess Emission in T Tauri Stars’, Astrophys. J. 382, 617–635.

    Article  ADS  Google Scholar 

  • Hartigan, P., Edwards, S., and Ghandour, L.: 1995, ‘Disk Accretion and Mass Loss from Young Stars’, Astrophys. J. 452, 736–768.

    Article  ADS  Google Scholar 

  • Hartmann, L.: 1998, ‘Accretion Processes in Star Formation’, Cambridge Univ. Press.

    Google Scholar 

  • Hartmann, L., and Kenyon, S. J.: 1996, ‘The FU Orionis Phenomenon’, Ann. Rev. Astron. Astrophys. 34, 207–240.

    Article  ADS  Google Scholar 

  • Hartmann, L., and Calvet, N.: 1995, ‘Observational Constraints on FU Ori Winds’, Astron. J. 109, 1846–1855.

    Article  ADS  Google Scholar 

  • Hartmann L., Hewett, R., and Calvet, N.: 1994, ‘Magnetospheric Accretion Models for T Tauri Stars. I: Balmer Line Profiles Without Rotation’, Astrophys. J. 426, 669–687.

    Article  ADS  Google Scholar 

  • Hartmann, L., Calvet, N., Gullbring, E., and D’Alessio, P. 1998, ‘Accretion and the Evolution of T Tauri Stars’, Astrophys. J. 495, 385–400.

    Article  ADS  Google Scholar 

  • Heyvaerts, J., Priest, E. R., and Bardou, A.: 1996, ‘Magnetic Field Diffusion in Self-consistently Turbulent Accretion Disks’, Astrophys. J. 473, 403–421.

    Article  ADS  Google Scholar 

  • Hirth, G. A., Mundt, R., and Solf, J.: 1997, ‘Spatial and Kinematic Properties of the Forbidden Emission Line Region of T Tauri Stars’, Astron. Astrophys. Suppl. 126, 437–469.

    Article  ADS  Google Scholar 

  • Jensen, E.L.N., Mathieu, R.D., and Fuller, G.A.: 1994, ‘A Connection Between Submillimeter Continuum Flux and Separation in Young Binaries’, Astrophys. J. 429, L29–L32.

    Article  ADS  Google Scholar 

  • Jensen, E.L.N., Mathieu, R.D., and Fuller, G. A.: 1996, ‘The Connection Between Submillimeter Continuum Flux and Binary Separation in Young Binaries: Evidence of Interaction Between Stars and Disks’, Astrophys. J. 458, 312–326.

    Article  ADS  Google Scholar 

  • Kenyon, S. J., and Hartmann, L.: 1987, ‘Spectral Energy Distributions of T Tauri Stars — Disk Flaring and Limits on Accretion’, Astrophys. J. 323, 714–733.

    Article  ADS  Google Scholar 

  • Kenyon, S. J., Hartmann, L. W.: 1991, ‘The Dusty Envelopes of FU Orionis Variables’, Astrophys. J. 383, 664–673.

    Article  ADS  Google Scholar 

  • Königl, A.: 1989, ‘Self-Similar Models of Magnetized Accretion Disks’, Astrophys. J. 342, 208–223.

    Article  ADS  Google Scholar 

  • Königl, A.: 1991, ‘Disk Accretion Onto Magnetic T Tauri Stars’, Astrophys. J. 370, L39–L43.

    Article  Google Scholar 

  • Kwan, J., and Tademaru, E.: 1995, ‘Disk Winds From T Tauri Stars’, Astrophys. J. 454, 382–393.

    Article  ADS  Google Scholar 

  • Meyer, M. R., Calvet, N., and Hillenbrand, L. A.: 1997, ‘Intrinsic Near-Infrared Excesses of T Tauri Stars: Understanding the Classical T Tauri Star Locus’, Astron. J. 114, 288–300.

    Article  ADS  Google Scholar 

  • Mundy, L.G., Looney, L.W., Erickson, W., Grossman, A., Welch, W.J., Forster, J.R., Wright, M.C.H., Plambeck, R.L., Lugten, J., and Thornton, D.D.: 1996, ‘Imaging the HL Tauri Disk at Lambda = 2.7 Millimeters with the BIMA Array’, Astrophys. J. 464, L169–L173.

    Article  ADS  Google Scholar 

  • Mundy, L. G., Looney, L. W., and Welch, W. J.: 2000, ‘The Structure and Evolution of Envelopes and Disks in Young Stellar Systems’, in V. Mannings, A.P. Boss, and S.S. Russell (eds.), Protostars and Planets IV, University of Arizona Press, Tucson, in press.

    Google Scholar 

  • Muzerolle, J., Hartmann, L., and Calvet, N. 1998, ‘A Br Gamma Probe of Disk Accretion in T Tauri Stars and Embedded Young Stellar Objects’, Astron. J. 116, 2965–2974.

    Article  ADS  Google Scholar 

  • Osterloh, M., and Beckwith, S.V.W.: 1995, ‘Millimeter-wave Continuum Measurements of Young Stars’, Astrophys. J. 439, 288–302.

    Article  ADS  Google Scholar 

  • Pollack, J. B., Hubickyj, O., Bodenheimer, P., Lissauer, J. J., Podolak, M., and Greenzweig, Y.: 1996, ‘Formation of the Giant Planets by Concurrent Accretion of Solids and Gas’, Icarus 124, 62–85.

    Article  ADS  Google Scholar 

  • Pudritz, R. E., and Norman, C.A.: 1983, ‘Centrifugally Driven Winds From Contracting Molecular Disks’, Astrophys. J. 274, 677–697.

    Article  ADS  Google Scholar 

  • Robert, F., Gauthier, D., and Dubrulle, B.: 2000, ‘The Solar System D/H Ratio: Observations and Theories’, Space Sci. Rev. 92, this volume.

    Google Scholar 

  • Rodriguez, L.F., D’Alessio, P., Wilner, D.J., Ho, P.T.P., Torrelles, J.M., Curiel, S., Gomez, Y., Lizano, S., Pedlar, A., Cantó, J., and Raga, A. C.: 1998, ‘Compact Protoplanetary Disks Around the Stars of a Young Binary System’, Nature 395, 355–357.

    Article  ADS  Google Scholar 

  • Shang, H., Shu, F.H., and Glassgold, A.E. 1998, ‘Synthetic Images and Long-slit Spectra of Protostellar Jets’, Astrophys. J. 493, L91–L94.

    Article  ADS  Google Scholar 

  • Shu, F., Najita, J., Ostriker, E., Wilkin, F., Rüden, S., and Lizano, S.: 1994a, ‘Magnetocentrifugally Driven Flows from Young Stars and Disks. 1: A Generalized Model’, Astrophys. J. 429, 781–796.

    Article  ADS  Google Scholar 

  • Shu, F. H., Najita, J., Ruden, S. P., and Lizano, S.: 1994b, ‘Magnetocentrifugally Driven Flows From Young Stars and Disks. 2: Formulation of the Dynamical Problem’, Astrophys. J. 429, 797–807.

    Article  ADS  Google Scholar 

  • Stapelfeldt, K., Burrows, C.J., Krist, J.E., and the WFPC2 science team: 1997, ‘Hubble Space Telescope Imaging of the Disks and Jets of Taurus Young Stellar Objects’, in B. Reipurth and C. Bertout (eds.), Herbig-Haro Flows and the Birth of Stars, IAU Symposium 182, Kluwer Academic Publishers, Dordrecht, pp. 355–364.

    Chapter  Google Scholar 

  • Stapelfeldt, K.R., Krist, J.E., Menard, F., Bouvier, J., Padgett, D.L., and Burrows, C. J.: 1998, ‘An Edge-On Circumstellar Disk in the Young Binary System HK Tauri’, Astrophys. J. 502, L65–L68.

    Article  ADS  Google Scholar 

  • Stepinski, T. F.: 1998, ‘The Solar Nebula as a Process — An Analytic Model’, Icarus 132, 100–112.

    Article  ADS  Google Scholar 

  • Stone, J.M., Hawley, J.F., Gammie, C.F., and Balbus, S.A.: 1996, ‘Three-dimensional Magnetohydrodynamical Simulations of Vertically Stratified Accretion Disks’, Astrophys. J. 463, 656–673.

    Article  ADS  Google Scholar 

  • Valenti, J. A., Basri, G., and Johns, C. M.: 1993, ‘T Tauri Stars in Blue’, Astron. J. 106, 2024–2050.

    Article  ADS  Google Scholar 

  • Zuckerman, B., Forveille, T., and Kastner, J. H.: 1995, ‘Inhibition of Giant Planet Formation by Rapid Gas Depletion Around Young Stars’, Nature 373, 494.

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

  1. Center for Astrophysics, 60 Garden St., Cambridge, MA, 02138, USA

    Lee Hartmann

Authors
  1. Lee Hartmann
    View author publications

    You can also search for this author in PubMed Google Scholar

Editor information

Editors and Affiliations

  1. Physikalisches Institut der Universität Bern, CH-3012, Bern, Switzerland

    W. Benz

  2. International Space Science Institute, CH-3012, Bern, Switzerland

    R. Kallenbach

  3. Kosmochemie, Max-Planck-Institut für Chemie, D-55020, Mainz, Germany

    G. W. Lugmair

Rights and permissions

Reprints and permissions

Copyright information

© 2000 Springer Science+Business Media Dordrecht

About this paper

Cite this paper

Hartmann, L. (2000). Observational Constraints on Transport (And Mixing) in Pre-Main Sequence Disks. In: Benz, W., Kallenbach, R., Lugmair, G.W. (eds) From Dust to Terrestrial Planets. Space Sciences Series of ISSI, vol 9. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4146-8_5

Download citation

  • DOI: https://doi.org/10.1007/978-94-011-4146-8_5

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-5807-0

  • Online ISBN: 978-94-011-4146-8

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics

Search

Navigation