Hostname: page-component-84b7d79bbc-2l2gl Total loading time: 0 Render date: 2024-07-27T19:24:11.741Z Has data issue: false hasContentIssue false
  • English
  • Français

Properties of the Winds of T Tauri Stars

Published online by Cambridge University Press:  25 May 2016

Nuria Calvet
Nuria Calvet*
Affiliation:
Centro de Investigaciones de Astronomía, Mérida, Venezuela, and Center for Astrophysics, 160 Concord, MA 02138, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The properties of Classical T Tauri (TTS) winds - their mass loss rate, temperature, origin, and energetics - are reviewed and interpreted in terms of the most recent observational evidence. TTS winds seem to have their origin in the disk and are powered by accretion. Most TTS have Ṁω ≤ 10–9Mʘ yr–1 and Ṁω/Ṁ ∼ 0.1, with T ∼ 104K.

Type
IV. Disks, Winds, and Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 182: Herbig-Haro Flows and the Birth of Low Mass Stars , 1997 , pp. 417 - 432
Copyright
Copyright © Kluwer 1997 

References

Appenzeller, I., Jankovics, I., Ostreicher, R.: 1984, AA, 141, 108.Google Scholar
Basri, G., Marcy, G. W., Valenti, J. A.: 1992, ApJ, 390, 622.Google Scholar
Blandford, R.D., Payne, D.G.: 1982, MNRAS 199, 883.Google Scholar
Bertout, C., Basri, G., Bouvier, J.: 1988, ApJ, 330, 350.Google Scholar
Bertout, C., Regev, O.: 1992, ApJ, 399, L163.CrossRefGoogle Scholar
Bacciotti, F., Hirth, G. A., Natta, A.: 1996, AA, 310, 309.Google Scholar
Cabrit, S., Edwards, S., Strom, S. E., Strom, K. M.: 1990, ApJ, 354, 687.Google Scholar
Calvet, N., Hartmann, L.: 1992, ApJ, 386, 239.Google Scholar
Calvet, N., Hartmann, L., Hewett, R.: 1992, ApJ, 386, 229.Google Scholar
Calvet, N., Magris C, G., Patiño, A., D'Alessio, P.: 1992, Rev. Mexicana AA, 24, 27.Google Scholar
Calvet, N., Hartmann, L., Kenyon, S. J.: 1993, ApJ, 402, 623.Google Scholar
Camenzind, M.: 1990, in Rev. Mod. Astron. 3, ed. Klare, G., Sringer-Verlag, 234.Google Scholar
Croswell, K., Hartmann, L., Avrett, E. H.: 1987, ApJ, 312, 227.Google Scholar
Edwards, S., Cabrit, S., Strom, S., Heyer, I., Strom, K. M., Anderson, E.: 1987, ApJ, 321, 473.Google Scholar
Edwards, S., Hartigan, P., Ghandour, L., Andrulis, C.: 1994, AJ, 108, 1056.Google Scholar
Folha, D., Emerson, J., Calvet, N.: 1997, Poster Proceedings of the IAU Symposium 182, eds. Malbet, F. and Castets, A., Observatoire de Grenoble, 272.Google Scholar
Giampapa, M. S., Basri, G., Johns, C. M., Imhoff, C. L. : 1993, ApJS, 89, 321.Google Scholar
Giovanardi, C., Gennari, S., Natta, A., Ruggero, S.: 1991, ApJ, 367, 173.Google Scholar
Ghosh, P., Lamb, F. K.: 1978, ApJ, 223, 83.Google Scholar
Gómez de Castro, A. I., Pudritz, R. E.: 1993, ApJ, 409, 748.Google Scholar
Gullbring, E., Hartmann, L., Briceño, C., Calvet, N.: 1997, in preparation.Google Scholar
Hamann, F.: 1994, ApJS, 93, 485.Google Scholar
Hartmann, L., Edwards, S., Avrett, E.: 1982, ApJ, 261, 279.Google Scholar
Hartmann, L., Raymond, J. C.: 1989, ApJ, 337, 903.Google Scholar
Hartmann, L., Calvet, N., Avrett, E. H., Loeser, R.: 1990, ApJ, 349, 168.CrossRefGoogle Scholar
Hartmann, L., Hewett, R., Calvet, N.: 1994, ApJ, 426, 669.Google Scholar
Hartmann, L., Kenyon, S. J.: 1996, ARAA, 34, 207.Google Scholar
Hartmann, L., Calvet, N.: 1995, AJ., 109, 1846.CrossRefGoogle Scholar
Hartmann, L.: 1997, Accretion Processes in Star Formation, Cambridge University Press.Google Scholar
Hartigan, P., Edwards, S., Ghandour, L.: 1995, ApJ, 452, 736 (HEG).Google Scholar
Hirth, G. A., Mundt, R., Solf, J.: 1993, AA, 285, 929.Google Scholar
Hirth, G. A., Mundt, R., Solf, J., Ray, T: 1994, ApJ, L99.Google Scholar
Holzer, E., Fla, T., Leer, E.: 1983, ApJ, 275, 808.Google Scholar
Jankovics, I., Appenzeller, I., Krautter, J.: 1983, PASP, 95, 883.CrossRefGoogle Scholar
Johns, C. M., Basri, G.: 1995a, ApJ, 449, 341.Google Scholar
Johns, C. M., Basri, G.: 1995b, AJ, 109, 2800.Google Scholar
Johns-Krull, C. M., Basri, G.: 1997, ApJ, 474, 433.Google Scholar
Kenyon, S. J., Hartmann, L.: 1987, ApJ, 323, 714.Google Scholar
Kepner, J., Hartigan, P., Yang, C., Strom, S.: 1993, ApJ, 415, L119.Google Scholar
Krautter, J., Appenzeller, I., Jankovics, I.: 1990, AA, 236, 416.Google Scholar
Königl, A.: 1989, ApJ, 342, 208.Google Scholar
Königl, A.: 1991, ApJ, 370, 39.Google Scholar
Kuhi, L. V.: 1964, ApJ, 140, 1409.CrossRefGoogle Scholar
Kwan, J., Tademaru, E.: 1988, ApJ, 332, L41.Google Scholar
Kwan, J., Tademaru, E.: 1995, ApJ, 454, 382.Google Scholar
Lago, M. T. V. T.: 1984, MNRAS, 210, 323.Google Scholar
Lago, M. T. V. T.: 1986, MNRAS, 222, 213.Google Scholar
Lynden-Bell, D., and Pringle, J. E.: 1974, MNRAS, 168, 603.Google Scholar
Mitskevich, A. S., Natta, A., Grinin, V. P.: 1993, ApJ, 404, 751.Google Scholar
Muzerolle, J., Calvet, N., Hartmann, L.: 1997, in preparation.Google Scholar
Najita, J. R., Shu, F. H.: 1994, ApJ, 429, 808.Google Scholar
Najita, J., Carr, J. S., Tokunaga, A. T.: 1996, ApJ, 456, 292.Google Scholar
Natta, A., Giovanardi, C.: 1990, ApJ, 356, 646.Google Scholar
Natta, A., Giovanardi, C., Palla, F.: 1988, ApJ, 332, 921.Google Scholar
Natta, A.: 1996, in ASP Conf. Proc. 109, Cool Stars, Stellar Systems and the Sun, eds. Pallavicini, R. and Dupree, A., (San Francisco: ASP), 471.Google Scholar
Ouyed, R., Pudritz, R. E.: 1994, ApJ, 423, 753.Google Scholar
Paatz, G., Camenzind, M.: 1996, AA, 308, 77.Google Scholar
Pelletier, G., Pudritz, R.E.: 1992, ApJ, 394, 117.Google Scholar
Petrov, P. P., Herbig, G. H.: 1992, ApJ, 392, 209.Google Scholar
Pringle, J. E.: 1989, MNRAS, 236, 107.Google Scholar
Pudritz, R.E., Norman, C.A.: 1983, ApJ, 274, 677.Google Scholar
Raga, A.: 1989, AJ, 98, 976.Google Scholar
Safier, P. N.: 1993, ApJ, 408, 148.Google Scholar
Shu, F. H., Najita, J. R., Ruden, S. P., Lizano, S.: 1994, ApJ, 429, 797.Google Scholar
Shu, F., Najita, J., Ostriker, E.C., Shang, H.: 1995, ApJ, 455, L155.Google Scholar
Solf, J., Böhm, K. H.: 1993, ApJ, L31.Google Scholar