Folha, Daniel - Centre for Astrophysics, University of Porto

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Folha, Daniel - Centre for Astrophysics, University of Porto

Line Profiles: Modeling The observational effort in obtaining high resolution hydrogen line spectra in T Tauri
Observations The observations presented in this work were carried out at the United Kingdom In
Data Reduction 3.1 General Procedure
Astron. Astrophys. 352, 517--531 (1999) ASTRONOMY ASTROPHYSICS
NEAR INFRARED LINES AS DIAGNOSTICS OF ACCRETION IN T TAURI STARS
Optical spectra of T Tauri stars often reveal their photospheric spectrum. For those stars spectral types have been determined using that information. However, many
Astronomy & Astrophysics manuscript no. (will be inserted by hand later)
Astronomy & Astrophysics manuscript no. ms18122col October 17, 2005 (DOI: will be inserted by hand later)
A&A 399, 271274 (2003) DOI: 10.1051/0004-6361:20021792
Line Profiles: Observations The Pafi and Brfl line profiles obtained for the observed T Tauri stars are presented in
Near Infrared Hydrogen Lines as Diagnostic of Accretion and Winds in Young Stellar Objects
A&A 388, 504517 (2002) DOI: 10.1051/0004-6361:20020413
Magnetospheric accretion and pre-main-sequence stellar masses Ian A. Bonnell,1
A&A 408, 10471055 (2003) DOI: 10.1051/0004-6361:20031011
Winds and Accretion in T Tauri Stars: Paschen Beta Line profiles