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Contents
List of Figures
List of Tables
Introduction
T Tauri Stars: Overview
Testing the Magnetospheric Accretion Model
Hydrogen Emission Lines in T Tauri Stars
Observations
UKIRT
CGS4
Data Acquisition
Setting Up Procedure
The CONFIG File
Taking Data
Observing an Astronomical Object
Sample of Observed T Tauri Stars
Observing Run: 1994
Observing Run: 1995
Data Reduction
General Procedure
Bad Pixel Masking
Bias Subtraction
Flat Fielding
Interleaving
Sky Subtraction
Optimal Extraction
De-rippling
Wavelength Calibration
Atmospheric Transmission and Instrumental Response
Flux Calibration
UT9410 Observing Run: Data Reduction
De-rippling
Wavelength Calibration
Atmospheric Transmission and Instrumental Response
Continuum Normalization
UT1295 Observing Run: Data Reduction
De-rippling
CVF Fringing
Wavelength Calibration
Atmospheric Transmission and Instrumental Response
Continuum Normalization
Noise Considerations
Velocity Scale
Spectra
Veiling
Computational Method
Choice of Template Star
Binaries and Veiling
Results
Discussion of Veiling Results
General Discussion
How Reliable are the Veiling Results?
Spectral Type Mismatch
(J-K) Colours
Comparison With Other Work
Conclusion
Line Profiles: Observations
Line Profile Classification
Line Parameters
Line Parameters: Computational Method
Line Parameters: Results
Statistics
Full Width at Half Maximum (FWHM)
Wing Maximum Velocity ( and )
Velocity of the Line Peak ()
Asymmetry Factor (Af)
The Type I Line Profiles
The Type II and Type III Line Profiles
The Type IV R Line Profiles
Discussion
Comparison with Accretion/Wind Models
The IPC Line Profiles
The Type I Line Profiles
Viewing Angle Effects
Multiple Systems
Comparison with other Pa /Br Line Profile Data
Line Profile Variability
Conclusion
Line Profiles: Modeling
Computational Method
CLOUDY
Line Profiles
Implementation
Input Parameters
Tests
Results
Wind Models
Accretion Models
Conclusions
Epilogue
Line Profiles
Veiling
Future Directions
Histograms: Method for Computation
Publications
References
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Daniel Folha
Fri Aug 28 11:53:21 BST 1998