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Pre-main sequence disks

Published online by Cambridge University Press:  27 April 2011

Gaspard Duchêne*
Affiliation:
Astronomy Department, University of California Berkeley, Berkeley CA 94720-3411, USA email: [email protected] Université Joseph Fourier - Grenoble 1/CNRS, Laboratoire d'Astrophysique de Grenoble (LAOG) UMR 5571, BP 53, 38041 Grenoble Cedex 09, France
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Abstract

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In this contribution, I briefly review our empirical knowledge of disks around ≲2M pre-main sequence (T Tauri) stars, focusing first on the dichotomic question of their frequency before moving on to some more detailed disk properties (overall orientation, total mass, outer radius). Finally, I conclude with a brief discussion of disks around embedded protostars, which will play in the next few years a major role in testing star formation theory and simulations.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Bouy, H., Huélamo, N., Pinte, C., Olofsson, J., Barrado y Navascués, D., Martín, E., Pantin, E., Monin, J. L., Basri, G., Augereau, J. C., Ménard, F., Duvert, G., Duchêne, G., Marchis, F., Bayo, A, Bottinelli, S., lefort, B., & Guieu, S. 2008, A&A, 486, 877Google Scholar
Enoch, M., Corder, S., Dunham, M., & Duchêne, G. 2009, ApJ, 707, 103CrossRefGoogle Scholar
Glauser, A., Ménard, F., Pinte, C., Duchêne, G., Güdel, M., Monin, J. L., & Padgett, D. 2008, A&A, 485, 531Google Scholar
Guarcello, M., Micela, G., Damiani, F., Peres, G., Prisinzano, L., & Sciortino, S. 2009, A&A, 496, 453Google Scholar
Hernández, J., Hartmann, L., Calvet, N., Jeffries, R., Gutermuth, R., Muzerolle, J., & Stauffer, J. 2008, ApJ, 686, 1195CrossRefGoogle Scholar
Hillenbrand, L., Strom, S., Calvet, N., Merril, M., Gatley, I., Makidon, R., Meyer, M., & Skutskie, M. 1998, AJ, 116, 1816CrossRefGoogle Scholar
Jörgensen, J., Bourke, T., Myers, P., Schöier, F., van Dishoeck, E., & Wilner, D. 2005, ApJ, 632, 973CrossRefGoogle Scholar
Kitamura, Y., Momose, M., Yokogawa, S., Kawabe, R., Tamura, M., & Ida, S. 2002, ApJ, 581, 357CrossRefGoogle Scholar
Luhman, K., Allen, P., Espaillat, C., Hartmann, L., & Calvet, N. 2010, ApJS, 186, 111CrossRefGoogle Scholar
Luhman, K., Adame, M., D'Alessio, P., Calvet, N., McLeod, K., Bohac, C., Forrest, W., Hartmann, L., Sargent, B., & Watson, D. 2007, ApJ, 666, 1219CrossRefGoogle Scholar
Maury, A., André, P., Hennebelle, P., Motte, F., Stamatellos, D., Bate, M., Belloche, A., Duchêne, G., & Whitworth, A. 2010, A&A, 512, 40Google Scholar
Ménard, F. & Duchêne, G. 2004, A&A, 425, 973Google Scholar
Mercer, E., Miller, J., Calvet, N., Hartmann, L., Hernández, J., Sicilia-Aguilar, A., & Gutermuth, R. 2009, ApJ, 138, 7CrossRefGoogle Scholar
Momose, M., Ohashi, N., Kudo, T., Tamura, M., & Kitamura, Y. 2010, ApJ, 712, 397CrossRefGoogle Scholar
Monin, J. L., Clarke, C., Prato, L., & McCabe, C. 2007, in: Reipurth, B., Jewitt, D., & Keil, K. (eds.), Protostars & Planets V, p. 395Google Scholar
Natta, A., Grinin, V., & Mannings, V. 2000, in: Mannings, V., Boss, A., & Russell, S. (eds.), Protostars & Planets IV, p. 559Google Scholar
Prato, L., Simon, M., Mazeh, T., Zucker, S., & McLean, I. 2002, ApJ (Letters), 579, L99CrossRefGoogle Scholar
Stapelfeldt, K., Krist, J., Ménard, F., Bouvier, J., Padgett, D., & Burrows, C. 1998, ApJ (Letters), 502, L65CrossRefGoogle Scholar
Tokovinin, A. 1997, A&AS, 124, 75Google Scholar
Watson, A., Stapelfeldt, K., Wood, K., & Ménard, F. 2007, in: Reipurth, B., Jewitt, D., & Keil, K. (eds.), Protostars & Planets V, p. 523Google Scholar