Computation of line and continuum radiation from thermal radioastronomical sources

Published: 1 January 1975| Version 1 | DOI: 10.17632/r6m4h6dw9x.1
M. Brocklehurst, M. Salem


Abstract Title of program: RCMBLN Catalogue number: AAEG Program obtainable from: CPC Program Library, Queen's University of Belfast, N. Ireland (see application form in this issue). Computer: IBM 360/65; Installation: University College London Computer Centre. Operating system: OS Programming language used: FORTRAN IV High speed storage required: 25000 words No. of bits in a word: 32 Overlay structure: None No. of magnetic tapes required: 2 (optional) Other peripherals used: Card reader, line printer... Title of program: RCMBLN Catalogue Id: AAEG_v1_0 Nature of problem The interpretation of radio recombination lines is of importance to radio astronomy. The computer program described in this paper calculates the intensities and profiles of hydrogen and helium radio recombination lines emitted by a thermal source. The electron temperature is assumed to be constant throughout the source,while the electron density is a known function of position. Spherical or plane parallel symmetry is assumed in the program. The theory of the method used is described in detail by ... Versions of this program held in the CPC repository in Mendeley Data aaeg_v1_0; RCMBLN; 10.1016/0010-4655(75)90012-0 This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2019)



Astronomy, Astrophysics, Computational Physics