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A multi-wavelength study of T Tauri stars

Title
A multi-wavelength study of T Tauri stars
Type
Article in International Conference Proceedings Book
Year
2001
Authors
Costa, VM
(Author)
Other
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Brooks, DH
(Author)
Other
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Gameiro, JF
(Author)
FCUP
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Conference proceedings International
Pages: 615-620
3rd 3-Island European Conference on Stellar Clusters and Associations - From Darkness to Light
CARGESE, FRANCE, APR 03-08, 2000
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Publicação em ISI Web of Knowledge ISI Web of Knowledge - 0 Citations
Scientific classification
FOS: Natural sciences > Physical sciences
Other information
Authenticus ID: P-000-X4M
Abstract (EN): We present results from a multi-wavelength study of T Tauri stars (TTS). This study is important for understanding the activity and evolution of young stars of different ages. Optical observations of blue/red-shifted absorption features are indicative of out/in-flows suggesting the presence of stellar winds and/or accretion. Constraints on the modelling are provided by the analysis of variability in the spectral features. The associated timescales have been used to differentiate between wind and infall regions and to help understand the boundary between out/in-flows around TTS. In addition, the UV spectroscopic analysis has recently been improved using collisional-radiative atomic models, resulting in more accurate determination of the atmospheric structure and physical properties of TTS and highlighting potential problems with the analysis methods. Our study of X-ray data has also revealed the connection between UV and X-ray emission which might be explained by solar-like coronal activity at a much higher level. Upcoming observations from XMM will allow a more complete examination of the detailed spectra.
Language: English
Type (Professor's evaluation): Scientific
No. of pages: 6
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