CO AND SHOCKS RELATED TO THE EVOLUTION OF THE ORION NEBULA
- 1 October 1982
- journal article
- Published by Wiley in Annals of the New York Academy of Sciences
- Vol. 395 (1) , 32-48
- https://doi.org/10.1111/j.1749-6632.1982.tb43376.x
Abstract
No abstract availableKeywords
This publication has 21 references indexed in Scilit:
- Structure and evolution of molecular clouds near H II regions. I - CO observations of an expanding molecular shell surrounding the Pelican NebulaThe Astrophysical Journal, 1980
- Molecular diagnostics of interstellar shocksThe Astrophysical Journal, 1980
- Spectrophotometry of quasi-stellar objects at optical and infrared wavelengths - PG 0026+129 and 3C 273The Astrophysical Journal, 1978
- Effects of expanding compact H II regions upon molecular clouds - Molecular dissociation waves, shock waves, and carbon ionizationThe Astrophysical Journal, 1978
- Molecular cooling and thermal balance of dense interstellar cloudsThe Astrophysical Journal, 1978
- The galactic density wave, molecular clouds, and star formationThe Astrophysical Journal, 1977
- On the molecular hydrogen emission at the Orion NebulaThe Astrophysical Journal, 1977
- Sequential formation of subgroups in OB associationsThe Astrophysical Journal, 1977
- Optical Emission from Shock Waves. II. Diagnostic DiagramsThe Astrophysical Journal Supplement Series, 1977
- The structure of the Orion nebulaPublications of the Astronomical Society of the Pacific, 1974