671 citations · 1k across the 6 of their papers we have counts for
6 papers
The [CII] 158 um Line Deficit in Ultraluminous Infrared Galaxies Revisited
M. L. Luhman, S. Satyapal, J. Fischer +5
We present a study of the [CII] 157.74 um fine-structure line in a sample of 15 ultraluminous infrared (IR) galaxies (L_IR>10^12 Lsun; ULIRGs) using the Long Wavelength Spectromete…
ISO-LWS spectroscopy of Centaurus A: extended star formation
S. J. Unger, P. E. Clegg, G. J. Stacey +9
We present the first full FIR spectrum of Centaurus A (NGC 5128) from 43 - 196.7 um. The data was obtained with the ISO Long Wavelength Spectrometer (LWS). We conclude that the FIR…
ISO Far-IR Spectroscopy of IR-Bright Galaxies and ULIRGs
J. Fischer, M. L. Luhman, S. Satyapal +16
Based on far-infrared spectroscopy of a small sample of nearby infrared-bright and ultraluminous infrared galaxies (ULIRGs) with the ISO Long Wavelength Spectrometer, we find a dra…
Far Infrared and Submillimeter Emission from Galactic and Extragalactic Photo-Dissociation Regions
Michael J. Kaufman, Mark G. Wolfire, David J. Hollenbach +1
Photodissociation Region (PDR) models are computed over a wide range of physical conditions, from those appropriate to giant molecular clouds illuminated by the interstellar radiat…
ISO LWS Spectroscopy of M82: A Unified Evolutionary Model
J. W. Colbert, M. A. Malkan, P. E. Clegg +9
We present the first complete far-infrared spectrum (43 to 197 um) of M82, the brightest infrared galaxy in the sky, taken with the Long Wavelength Spectrometer of the Infrared Spa…
Near-Infrared Spectroscopy of Photodissociation Regions: The Orion Bar and Orion S
K. L. Luhman, C. W. Engelbracht, M. L. Luhman
To test the PDR model spectra under the physical conditions present in Orion, we have obtained moderate-resolution (R=3000) J-, H-, and K-band long-slit spectra of the Orion bar an…