A computer program for fast non-LTE analysis of interstellar line spectra

Free access article

Issue		A&A Volume 468, Number 2, June III 2007


Page(s)		627 - 635
Section		Interstellar and circumstellar matter
DOI		http://dx.doi.org/10.1051/0004-6361:20066820

A&A 468, 627-635 (2007)
DOI: 10.1051/0004-6361:20066820

With diagnostic plots to interpret observed line intensity ratios

F. F. S. van der Tak^{1, 2}, J. H. Black³, F. L. Schöier⁴, D. J. Jansen⁵, and E. F. van Dishoeck⁵

¹ Netherlands Institute for Space Research (SRON), Landleven 12, 9747 AD Groningen, The Netherlands
e-mail: vdtak@sron.rug.nl
² Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
³ Onsala Space Observatory, Chalmers University of Technology, 43992 Onsala, Sweden
⁴ Stockholm Observatory, AlbaNova University Center, 10691 Stockholm, Sweden
⁵ Leiden University Observatory, PO Box 9513, 2300 RA Leiden, The Netherlands

(Received 27 November 2006 / Accepted 27 March 2007)

Abstract
Aims.The large quantity and high quality of modern radio and infrared line observations require efficient modeling techniques to infer physical and chemical parameters such as temperature, density, and molecular abundances.
Methods.We present a computer program to calculate the intensities of atomic and molecular lines produced in a uniform medium, based on statistical equilibrium calculations involving collisional and radiative processes and including radiation from background sources. Optical depth effects are treated with an escape probability method. The program is available on the World Wide Web at http://www.sron.rug.nl/~vdtak/radex/index.shtml. The program makes use of molecular data files maintained in the Leiden Atomic and Molecular Database (LAMDA), which will continue to be improved and expanded.
Results.The performance of the program is compared with more approximate and with more sophisticated methods. An Appendix provides diagnostic plots to estimate physical parameters from line intensity ratios of commonly observed molecules.
Conclusions.This program should form an important tool in analyzing observations from current and future radio and infrared telescopes.

Key words: radiative transfer -- methods: numerical -- radio lines: ISM -- infrared: ISM -- submillimeter

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