Published December 15, 1984 | Version v1
Journal article

Jet deflection and hairpin bends

Creators

  • 1. Maryland Univ., College Park (USA)

Description

The deflection of a hydrodynamic jet via an oblique internal shock is studied. The pressure increase across the shock and the confinement of the shocked jet are maintained by the ramming of the bend through the ambient medium. A steady flow pattern is found in the reference frame co-moving with the bend: the external ram pressure gradually bends the deflected jet by up to 1800. The shock polar method is used to quantify this model and it is found that changes in the initial angle of deflection and fluid dynamic instabilities will destroy this flow pattern for heavy jets. The model is applied to the U-shaped channels in the radio galaxies 3C 401 and 4C 32.69 and the head-tail source IC 708. (author)

Additional details

Publishing Information

Journal Title
Mon. Not. R. Astron. Soc.
Journal Volume
211
Journal Issue
4
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
767-773
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
16032573
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BENDING; GAS FLOW; HYDRODYNAMIC MODEL; INTERGALACTIC SPACE; JETS; RADIO GALAXIES; SHOCK WAVES
Descriptors DEC
COSMIC RADIO SOURCES; DEFORMATION; FLUID FLOW; GALAXIES; MATHEMATICAL MODELS; PARTICLE MODELS; SPACE; STATISTICAL MODELS; THERMODYNAMIC MODEL