M
M. L. Luhman
Researcher at United States Naval Research Laboratory
Publications - 12
Citations - 2223
M. L. Luhman is an academic researcher from United States Naval Research Laboratory. The author has contributed to research in topics: Galaxy & Photodissociation region. The author has an hindex of 9, co-authored 12 publications receiving 2150 citations. Previous affiliations of M. L. Luhman include Institute for Defense Analyses.
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Journal ArticleDOI
Far-Infrared and Submillimeter Emission from Galactic and Extragalactic Photodissociation Regions
TL;DR: In this article, the effects of metallicity and cloud extinction on the predicted line intensities were examined for a wide range of physical conditions, from those appropriate to giant molecular clouds illuminated by the interstellar radiation field to the conditions experienced by circumstellar disks very close to hot massive stars.
Journal ArticleDOI
Far Infrared and Submillimeter Emission from Galactic and Extragalactic Photo-Dissociation Regions
TL;DR: In this article, the effects of metallicity and cloud extinction on the predicted line intensities were examined for PDR models with densities over the range n=10^1-10^7 cm^-3.
Journal ArticleDOI
The [C II] 158 micron line deficit in ultraluminous infrared galaxies revisited
M. L. Luhman,M. L. Luhman,Shobita Satyapal,Shobita Satyapal,J. Fischer,Mark G. Wolfire,Eckhard Sturm,C. C. Dudley,Dieter Lutz,R. Genzel +9 more
TL;DR: In this article, the authors present a study of the [C II] 157.74 μm fine-structure line in a sample of 15 ultraluminous infrared (IR) galaxies using the Long Wavelength Spectrometer (LWS) on the Infrared Space Observatory (ISO).
Journal ArticleDOI
The [CII] 158 um Line Deficit in Ultraluminous Infrared Galaxies Revisited
M. L. Luhman,Shobita Satyapal,J. Fischer,Mark Wolfire,Eckhard Sturm,C. C. Dudley,Dieter Lutz,R. Genzel +7 more
TL;DR: In this article, Luhman et al. presented a study of the [CII] 157.74 um fine-structure line in a sample of 15 ultraluminous infrared (IR) galaxies using the Long Wavelength Spectrometer (LWS) on the Infrared Space Observatory (ISO).
Journal ArticleDOI
Infrared Space Observatory Measurements of a [C II] 158 micron Line Deficit in Ultraluminous Infrared Galaxies
M. L. Luhman,Shobita Satyapal,Jacqueline Fischer,Mark G. Wolfire,Mark G. Wolfire,Pierre Cox,S. D. Lord,Howard A. Smith,Gordon J. Stacey,S. J. Unger +9 more
TL;DR: In this paper, the authors reported measurements of the 157.74 μm fine-structure line in a sample of seven ultraluminous infrared galaxies (ULIGs) (LIR > 1012 L☉) with the Long Wavelength Spectrometer on the Infrared Space Observatory.