ILTHII — Analysis of the spectrum of a thermal radioastronomical source

Published: 1 January 1975| Version 1 | DOI: 10.17632/36zbjcf4fn.1
M. Salem


Abstract Title of program: ILTHII Catalogue number: AAEF 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: 24000 words. No. of bits in a word: 32 Overlay structure: Overlaid (29000 words required if not overlaid) No. of magnetic tapes required: None Other peripher... Title of program: ILTHII Catalogue Id: AAEF_v1_0 Nature of problem It has been shown by Salem and Seaton that, given the spectrum of a thermal radioastronomical source, information on the structure can be deduced in the form of a function Omega(E), which is the total angular area within which the emission measure is greater than or equal to E. A spherical model of the object can also be constructed. An estimate of the electron temperature, Te, (assumed to be constant) is required. In some cases this estimate may be improved by comparing Omega(E) with observatio ... Versions of this program held in the CPC repository in Mendeley Data AAEF_v1_0; ILTHII; 10.1016/0010-4655(75)90011-9 This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2019)



Astronomy, Astrophysics, Computational Physics