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