New determinations of the critical velocities of C-type shock waves in dense molecular clouds: application to the outflow source in Orion
Open Access
- 1 June 2002
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 332 (4) , 985-993
- https://doi.org/10.1046/j.1365-8711.2002.05373.x
Abstract
No abstract availableKeywords
This publication has 28 references indexed in Scilit:
- VODE: A Variable-Coefficient ODE SolverSIAM Journal on Scientific and Statistical Computing, 1989
- The velocity profile of the 1 - 0 S(1) line of molecular hydrogen at Peak 1 in OrionMonthly Notices of the Royal Astronomical Society, 1989
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989
- The rate of dissociation of molecular hydrogen by hydrogen atoms at very low densitiesThe Astrophysical Journal, 1986
- The Lyman and Werner bands of H2Canadian Journal of Physics, 1984
- The 1D-3P transition in atomic oxygen induced by collisions with atomic hydrogenThe Astrophysical Journal, 1983
- Magnetohydrodynamic shock waves in molecular cloudsThe Astrophysical Journal, 1983
- Molecular shock waves in the BN-KL region of OrionThe Astrophysical Journal, 1982
- A model for the intense molecular line emission from OMC-1The Astrophysical Journal, 1982
- Collisions of Electrons with Hydrogen Atoms. I. IonizationPhysical Review B, 1958