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- ASTRA
- acronym meaning
- Introduction
- convergence check
- Convergence Check
- flow diagram
- The STENHOLM Method
- intersect array
- Calculating the lines of
| The midfind subroutine
- line of sight
- co-ordinate system for output
- Define the line of
- for telescope
- Define the line of
- lines of sight
- Calculating the lines of to Calculating the lines of
- testing
- Testing the geometry section to Testing the geometry section
- output example
- Outputting the Results
- ring labelling
- Ring parameter calculations
- setup
- Using the Tcl/Tk Interface to mcs Files
- input/output files
- Input/Output Files for the to mcs Files
- outflow
- Using the Tcl/Tk Interface
- testing
- Testing the ASTRA program to Test Summary
- Buckley model
- A Detailed Comparison with
| A Detailed Comparison with
| Solid Body Rotation
- inner cut off values
- A Detailed Comparison with
- Krügel & Chini model
- A Detailed Comparison with
- LVG case
- The LVG case
| The LVG case
- Richer and Padman
- Keplerian Rotation to Keplerian Rotation
- ring numbers
- A Detailed Comparison with
- solid body rotation
- Solid Body Rotation
- using dust model
- A Subjective Test Using
- velocity types
- Calculating the ring relative
| run.** (19)
- velocity vectors
- Relative velocity between two
- Buckley
- A Detailed Comparison with
| A Detailed Comparison with
| Solid Body Rotation
- collision coefficients
- Statistical Equilibrium
- Einstein coefficients
- Einstein Coefficients
| Source of the Einstein
- Hildebrand dust model
- A Modification to Allow
- JCMT
- description of
- The James Clerk Maxwell
- lines of sight
- interpolation method
- Solving the Radiative Transfer
- interpolation problems
- Solving the Radiative Transfer
- LVG
- The LVG Approximation
| The LVG case
- molecules
- types
- The Theory Of Spectral
- protostar
- classification
- Classification of Protostellar Objects
- formation of
- From Clump to Protostar
- radiative transfer
- co-moving frame
- The STENHOLM Method
- computer solution
- Solving the Radiative Transfer
- core saturation
- The STENHOLM Method
- equation
- Solving the Radiative Transfer
- Feautrier
- The Feautrier Method
- LVG method
- The LVG Approximation
- Monte Carlo method
- The Monte Carlo Method
- Stenholm
- The STENHOLM Method
- Richer and Padman
- Keplerian Rotation to Keplerian Rotation
- rotation diagram
- Rotation Diagrams
- source function
- The Source Function
- spectral line
- theory
- The Theory Of Spectral to The Theory Of Spectral
- transition
- CN
- The Theory Of Spectral
| The Theory Of Spectral
- CO
- The Theory Of Spectral
- lettering convention
- The Theory Of Spectral
- star formation
- stages of
- The Stages of Star
- STEN
- example output
- Summary of Thesis Contents
- H
CO example
- An Example Using the
- how to use
- Initial setup to Other files
- new features
- New features
- non-linear molecule handelling
- Re-labelling the Data Arrays
- shell distribution
- Setting up the model
- telescope beam
- convolution
- Gridded convolution
- temperature
- brightness
- The radiative transfer equation
- radiation
- The radiative transfer equation
- T
- Correcting the Temperature Scale
1999-04-12