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39 lines (39 loc) · 1.35 KB
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cff-version: 1.2.0
message: "If you use SimLine in published research, please cite it as below."
title: SimLine
abstract: >
SimLine is a FORTRAN code for computing molecular transition line profiles
in spherically symmetric clouds with arbitrary density, temperature and
velocity structure. Turbulence and clumping are treated in a local
statistical approximation with a radial dependence of the correlation
parameters. The code solves the radiative transfer and level population
equations self-consistently using an accelerated lambda iteration and
computes emergent line profiles convolved with a Gaussian telescope beam.
version: "2.18"
license: GPL-3.0-or-later
authors:
- family-names: Ossenkopf-Okada
given-names: Volker
affiliation: "I. Physikalisches Institut, Universität zu Köln"
email: ossk@ph1.uni-koeln.de
preferred-citation:
type: article
title: "Massive core parameters from spatially unresolved multi-line observations"
authors:
- family-names: Ossenkopf
given-names: Volker
- family-names: Trojan
given-names: Christoph
- family-names: Stutzki
given-names: Jürgen
journal: "Astronomy & Astrophysics"
volume: 378
start: 608
year: 2001
repository-code: "https://github.com/[owner]/simline"
keywords:
- radiative transfer
- molecular lines
- astrophysics
- interstellar medium
- FORTRAN