Published April 1975
| Version v1
Journal article
Accretion and effluxion of mass and angular momentum
Description
The hydrodynamical accretion and effiuxion of isentropic or isothermal material with uniform specific angular momentum, L sin θ, is solved exactly on a stream line, θ = constant. The critical value for L, Lm(γ), above which accretion is severely curtailed and effiuxion is rotationally driven, is found as the principal new result. This critical value appears as the maximum L for which Venturi flow (i.e. with a choke point) occurs. The accretion-effiuxion rate, A, and the location of the choke point, R, are given exactly for the Venturi curves as a function of L. The topology of the solutions is shown to include a vortex (elliptic) point as well as a choke (hyperbolic) point, and the figures display this behaviour explicitly.
Additional details
Identifiers
Publishing Information
- Journal Title
- Monthly Notices of the Royal Astronomical Society
- Journal Volume
- 171
- Journal Issue
- 1
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 27-34
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 6193597
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANGULAR MOMENTUM; BINARY STARS; COSMOLOGICAL MODELS; HYDRODYNAMICS; MASS TRANSFER; STAR ACCRETION
- Descriptors DEC
- FLUID MECHANICS; MATHEMATICAL MODELS; MECHANICS; STAR EVOLUTION; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent