Published February 15, 1991
| Version v1
Journal article
Shock absorbers in bipolar outflows
- 1. Edinburgh Univ. (UK). Dept. of Astronomy
- 2. Durham Univ. (UK). Dept. of Physics
- 3. Manchester Univ. (UK). Inst. of Science and Technology
Description
A type of shock which accelerates hydrogen molecules to a high velocity without dissociating is investigated. Such soft C-shocks are characterized by low Alfven Mach numbers and low streaming speed of the ions through the neutrals. Therefore, a shock in a region of high Alfven speed, υA can produce wide H2 line profiles. We show that the shape and width of the H2 line profiles in the OMC-1 outflow are reproduced by a bow shock of velocity 200-250 km s-1 moving through a dense medium with υA∼46 km s-1. Line ratio data are also successfully modelled from which we infer an H2O abundance <2x10-4 per hydrogen atom, within the shock. (author)
Additional details
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 248
- Journal Issue
- 4
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 730-740
- ISSN
- 0035-8711
- CODEN
- MNRAA
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 22057908
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ABSORPTION; ALFVEN WAVES; COSMIC GASES; GAS FLOW; HYDROGEN; LINE WIDTHS; MOLECULES; SHOCK WAVES; SIMULATION
- Descriptors DEC
- ELEMENTS; FLUID FLOW; FLUIDS; GASES; HYDROMAGNETIC WAVES; NONMETALS