Magnetospheric Accretion Models for the Hydrogen Emission Lines of T Tauri Stars
- 10 January 1998
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 492 (2) , 743-753
- https://doi.org/10.1086/305069
Abstract
No abstract availableThis publication has 27 references indexed in Scilit:
- Disk Accretion and Mass Loss from Young StarsThe Astrophysical Journal, 1995
- Spectroscopic evidence for magnetospheric accretion in classical T Tauri starsThe Astronomical Journal, 1994
- Emission-line studies of young stars. I - The T Tauri stars. II - The Herbig Ae/Be starsThe Astrophysical Journal Supplement Series, 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
- Optical excess emission in T Tauri starsThe Astrophysical Journal, 1991
- Winds from T Tauri stars. I - Spherically symmetric modelsThe Astrophysical Journal, 1990
- Accretion disks around T Tauri starsThe Astrophysical Journal, 1988
- Stellar winds and molecular clouds - Herbig Be and AE type starsThe Astrophysical Journal, 1984
- Line profiles in the YY Orionis star S Coronae AustrinaePublications of the Astronomical Society of the Pacific, 1979