Near-infrared echelle spectroscopy of Class I protostars: molecular hydrogen emission-line (MHEL) regions revealed
Open Access
- 1 September 2001
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 326 (2) , 524-538
- https://doi.org/10.1046/j.1365-8711.2001.04560.x
Abstract
No abstract availableKeywords
This publication has 72 references indexed in Scilit:
- Profiles of Strong Permitted Lines in Classical T Tauri StarsThe Astronomical Journal, 2000
- The Structure of Protostellar Envelopes Derived from Submillimeter Continuum ImagesThe Astrophysical Journal, 2000
- A Parsec‐Scale Herbig‐Haro Jet in Barnard 5The Astrophysical Journal, 1996
- Bolometric temperature and young stars in the Taurus and Ophiuchus complexesThe Astrophysical Journal, 1995
- The H2 velocity field in Herbig-Haro 7-11The Astrophysical Journal, 1993
- Winds from T Tauri stars. II - Balmer line profiles for inner disk windsThe Astrophysical Journal, 1992
- Measurements of Br-gamma and H2 in young stellar objectsThe Astronomical Journal, 1990
- Near-infrared CO emission in young stellar objectsThe Astrophysical Journal, 1989
- The formation of solar type stars - IRAS observations of the dark cloud Barnard 5The Astrophysical Journal, 1984
- Line positions and strengths in the H2 quadrupole spectrumThe Astrophysical Journal, 1982