Properties of the Winds of T Tauri Stars
- 1 January 1997
- book chapter
- Published by Springer Nature
Abstract
No abstract availableKeywords
This publication has 51 references indexed in Scilit:
- Mass loss from pre-main-sequence accretion disks. I - The accelerating wind of FU OrionisThe Astrophysical Journal, 1993
- Cool mass-losing boundary layers of T Tauri accretion disksThe Astrophysical Journal, 1992
- Limits on the magnetic flux of pre-main-sequence starsThe Astrophysical Journal, 1992
- Balmer line profiles for infalling T Tauri envelopesThe Astrophysical Journal, 1992
- Winds from T Tauri stars. II - Balmer line profiles for inner disk windsThe Astrophysical Journal, 1992
- Forbidden-line emission and infrared excesses in T Tauri stars - Evidence for accretion-driven mass loss?The Astrophysical Journal, 1990
- Accretion disks around T Tauri starsThe Astrophysical Journal, 1988
- Forbidden line and H-alpha profiles in T Tauri star spectra - A probe of anisotropic mass outflows and circumstellar disksThe Astrophysical Journal, 1987
- Mass loss from FU Orionis objectsThe Astrophysical Journal, 1987
- Hydromagnetic flows from accretion discs and the production of radio jetsMonthly Notices of the Royal Astronomical Society, 1982