Dust Emission from L1641N: An Optically Thick Circumstellar Disk?
- 10 September 1995
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 450 (2) , L71-L74
- https://doi.org/10.1086/316773
Abstract
No abstract availableThis publication has 17 references indexed in Scilit:
- Infrared CO Emission from Young Stars: Accretion Disks and Neutral WindsThe Astrophysical Journal, 1995
- Reassessment of millimetre-wave absorption coefficients in interstellar silicate grainsNature, 1994
- Protostellar accretion disks resolved with the JCMT-CSO interferometerThe Astrophysical Journal, 1994
- Infrared and optical imaging of IRAS sources with CO outflow - A snapshot of early star formationThe Astrophysical Journal, 1993
- Particle emissivity in circumstellar disksThe Astrophysical Journal, 1991
- Submillimeter photometry and disk masses of T Tauri disk systemsThe Astrophysical Journal, 1990
- Forbidden line and H-alpha profiles in T Tauri star spectra - A probe of anisotropic mass outflows and circumstellar disksThe Astrophysical Journal, 1987
- Spectral evolution of young stellar objectsThe Astrophysical Journal, 1987
- Discovery of seven bipolar outflows by an unbiased surveyThe Astrophysical Journal, 1986
- Optical properties of interstellar graphite and silicate grainsThe Astrophysical Journal, 1984