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Photoionization modeling of the LWS fine-structure lines in IR bright galaxiesThe long wavelength spectrometer (LWS) fine structure line spectra from infrared luminous galaxies were modeled using stellar evolutionary synthesis models combined with photoionization and photodissociation region models. The calculations were carried out by using the computational code CLOUDY. Starburst and active galactic nuclei models are presented. The effects of dust in the ionized region are examined.
Document ID
19980218764
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Satyapal, S. (NASA Goddard Space Flight Center Greenbelt, MD United States)
Luhman, M. L. (Naval Research Lab. Washington, DC United States)
Fischer, J. (Naval Research Lab. Washington, DC United States)
Greenhouse, M. A. (NASA Goddard Space Flight Center Greenbelt, MD United States)
Wolfire, M. G. (Maryland Univ. College Park, MD United States)
Date Acquired
August 18, 2013
Publication Date
December 1, 1997
Publication Information
Publication: Proceedings of the 1st ISO Workshop on Analytical Spectroscopy
Publisher: European Space Agency. European Space Research and Technology Center, ESTEC
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
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