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Primeval Jets from Young Stars

Published online by Cambridge University Press:  21 October 2010

T. P. Ray
T. P. Ray*
Affiliation:
Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland email: [email protected]
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Abstract

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The jet phenomenon lasts at least a million years for young, solar-like, stars and it occurs during a wide variety of young stellar object (YSO) phases. This includes the period when the source is highly embedded (Class 0) to when it becomes optically visible for the first time as a classical T Tauri star (Class II). Here I briefly discuss some of the properties of jets from the youngest objects.

Keywords

ProtostarYSOjetaccretionoutflowHerbig-Haro objectinterstellar medium
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 241 - 242
Copyright
Copyright © International Astronomical Union 2010

References

Caratti, o, Garatti, A., Eislöffel, J., Froebrich, D., Nisini, B., Giannini, T., & Calzoletti, L. 2009, A&A, 502, 579Google Scholar
Dionatos, O., Nisini, B., Garci ALopez, R., Giannini, T., Davis, C. J., Smith, M. D., Ray, T. P., & DeLuca, M. 2009, ApJ, 692, 1CrossRefGoogle Scholar
Evans, N. J., et al. 2009, ApJS, 181, 321CrossRefGoogle Scholar
Jones, A. P., Tielens, A. G. G. M., Hollenbach, D. J., & McKee, C. F. 1994, ApJ, 433, 797CrossRefGoogle Scholar
Kirk, J. M., Ward-Thompson, D., & André, P. 2007, MNRAS, 375, 843CrossRefGoogle Scholar
Lee, C.-F., Hirano, N., Palau, A., Ho, P. T. P., Bourke, T. L., Zhang, Q., & Shang, H. 2009, ApJ, 699, 1584CrossRefGoogle Scholar
Podio, L., Medves, S., Bacciotti, F., Eislöffel, J., & Ray, T. P. 2009, arXiv:0907.3842Google Scholar
Robitaille, T. P., Whitney, B. A., Indebetouw, R., Wood, K., & Denzmore, P. 2006, ApJS, 167, 256CrossRefGoogle Scholar