Line formation in the inner winds of classical T Tauri stars: testing the conical-shell wind solution
Article first published online: 17 OCT 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 426, Issue 4, pages 2901–2916, 11 November 2012
How to Cite
Kurosawa, R. and Romanova, M. M. (2012), Line formation in the inner winds of classical T Tauri stars: testing the conical-shell wind solution. Monthly Notices of the Royal Astronomical Society, 426: 2901–2916. doi: 10.1111/j.1365-2966.2012.21853.x
- Issue published online: 17 OCT 2012
- Article first published online: 17 OCT 2012
- Manuscript Accepted: 1 AUG 2012
- Manuscript Received: 26 JUL 2012
- NASA. Grant Numbers: NNX10AF63G, NNX11AF33G
- NSF. Grant Number: AST-1008636
- NASA High-End Computing (HEC)
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