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Disks Around T Tauri Stars

Published online by Cambridge University Press:  12 April 2016

Anneila Sargent  and
Steven Beckwith
Anneila Sargent
Affiliation:
Division of Physics, Mathematics, & Astronomy, California Institute of Technology, Pasadena, CA, USA 91125
Steven Beckwith
Affiliation:
Max Planck Institut für Astronomie, Kõnigstuhl 17, W-6900 Heidelberg, Federal Republic of Germany

Abstract

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A variety of evidence suggests that at least 50% of T Tauri stars are surrounded by disks of gas and dust. Inferred disk properties are compatible with those generally attributed to the solar nebula, before the formation of planets. Millimeter-wave aperture synthesis mapping of molecular line and dust continuum emission from T Tauri stars provides a direct way to ascertain if disks are present. The technique enables detailed studies of disk temperature and density distributions, chemical properties and velocity fields. These results inform our understanding of both star formation and solar system evolution. We review the observations to date and discuss directions for future research.

Type
3. Astronomical Results and Prospects
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 203 - 211
Copyright
Copyright © Astronomical Society of the Pacific 1994

References

Adams, F.C., Emerson, J.P., & Fuller, G.A. 1990, ApJ, 357, 606.CrossRefGoogle Scholar
Adams, F.C., Lada, C.J. & Shu, F.H. 1988, ApJ, 326, 865.Google Scholar
Adams, F.C., Ruden, S.P. & Shu, F.H. 1989, ApJ, 347, 959.Google Scholar
Appenzeller, I. & Mundt, R. 1989, A&A Rev., 1, 291.Google Scholar
Barshay, S.S., & Lewis, J.S. 1976, ARA&A, 14, 81.Google Scholar
Bastian, U., Finkenzeller, U., Jascheck, C., & Jascheck, M. 1983, A&A, 126 438.Google Scholar
Beckwith, S.V.W., & Sargent, A.I. 1992a, in Protostars and Planets HI, ed. Levy, E. H., Lunine, J.I. & Matthews, M. S. (Tucson:University of Arizona Press), in press.Google Scholar
Beckwith, S.V.W., & Sargent, A.I. 1992b, ApJ, in press.Google Scholar
Beckwith, S.V.W., Sargent, A.I., Chini, R., & Gusten, R. 1990, AJ, 99, 924 BSCG. Google Scholar
Beckwith, S., Sargent, A.L., Scoville, N.Z., Masson, C.R., Zuckerman, B., & Phillips, T.G. 1986, ApJ, 309, 755.CrossRefGoogle Scholar
Bertout, C. 1989, ARA&A, 27, 351.Google Scholar
Bieging, J.H., Cohen, M., & Schwartz, P.R. 1984, ApJ, 282, 699.Google Scholar
Blake, G.A., van Dishoeck, E.F., & Sargent, A.I. 1992, ApJ, 391, L99.Google Scholar
Bonnell, L., Martel, H., Bastien, P., Arcoragi, J., & Benz, W. 1991, ApJ, 377, 553.Google Scholar
Clarke, C. J., & Pringle, J. E. 1991, MNRAS, 249, 588.CrossRefGoogle Scholar
Cohen, M., & Kuhi, L.V. 1979, ApJS, 41, 743.CrossRefGoogle Scholar
Edwards, S., Ray, T.P., & Mundt, R. 1992, in Protostars & Planets IH, ed. Levy, E. H., Lunine, J.I., & Matthews, M. S. (Tucson:University of Arizona Press), in press.Google Scholar
Ghez, A. 1992, Ph. D. Thesis, California Institute of Technology.Google Scholar
Herbig, G.H. 1962, Adv. A&A, 1, 147.Google Scholar
Joy, A.H. 1945, ApJ, 102, 168.CrossRefGoogle Scholar
Koerner, D.W., Sargent, A. L., & Beckwith, S.V.W. ApJ, submitted.Google Scholar
Leinert, Ch. Haas, M., Richichi, A., Zinnecker, H., & Mundt, R. 1991, A&A, 250, 407.Google Scholar
Leinert, Ch., Weitzel, N., Haas, M., Lenzen, R., Zinnecker, H., Christou, J., Ridgway, S., Jameson, R., & Richichi, A. 1992, A&A, in press.Google Scholar
Lin, D.N.C., & Papaloizou, J. 1985, in Protostars & Planets II, ed. Black, D. C. & Matthews, M. S. (Tuscon: University of Arizona Press), 981.Google Scholar
Mathieu, R.D. 1992, in IAU Symposium No. 151, Interacting Binary Stars, eds. Kondo, Y. & Polidan, R. (Dordrecht:Reidel), in press.Google Scholar
Mundt, R. 1988, in NATO-ASI on Formation & Evolution of Low Mass Stars, eds. Dupree, A. K. & Lago, M. T. V. T. (Dodrecht:Kluwer), 257.Google Scholar
Mundt, R., Ray, T.P. & Bührke, T. 1988, ApJ, 333, L69.Google Scholar
Ohashi, N., Kawabe, R., Hayashi, M., & Ishiguro, H. 1991, AJ., 102, 2054.Google Scholar
Omodaka, T., Kitamura, Y., & Kawazoe, E. 1992, ApJ, 396, L87.Google Scholar
Safronov, V.S., & Ruzmaikina, T.V. 1985, in Protostars &, Planets II, ed. Black, D. C. & Matthews, M. S. (Tucson:University of Arizona Press), 959.Google Scholar
Sargent, A.I. & Beckwith, S.V.W., 1987, ApJ, 323, 294.Google Scholar
Sargent, A.L., & Beckwith, S.V.W. 1989, in I. A. U. Colloquium No. 120, “Structure and Dynamics of the Interstellar Medium”, ed. Tenorio-Tagle, G., Melnick, J., & Moles, M. (Springer-Verlag:Berlin), 221.Google Scholar
Sargent, A.I. & Beckwith, S.V.W., 1991, ApJ, 382, L31.Google Scholar
Shu, F.H., Adams, F.C., & Lizano, S. 1987, ARA&A, 25, 23.Google Scholar
Shu, F.A., Najita, J., Galli, D., & Ostriker, E. 1992, in Protostars & Planets IH, ed. Levy, E. H., Lunine, J.I., & Matthews, M. S. (Tucson:University of Arizona Press), in press.Google Scholar
Simon, M., Chen, W.P., Howell, R.R., Benson, J.A., & Słowik, D. 1992, ApJ, 384, 212.CrossRefGoogle Scholar
Simon, M., & Guilloteau, S. 1992, ApJ. 397, L47.Google Scholar
Strom, K.M., Strom, S.E., Edwards, S., Cabrit, S., & Skrutskie, M.F. 1989, AJ, 97, 1451.Google Scholar
Weintraub, D.A., Masson, C.R., & Zuckerman, B. 1989, ApJ, 344, 915.CrossRefGoogle Scholar