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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…
A Narrowband Imaging Search for [OIII] Emission from Galaxies at z>3
Harry I. Teplitz, Matthew A. Malkan, Ian S. McLean
We present the results of a narrow-band survey of QSO fields at redshifts that place the [OIII](5007) emission line in the 1% 2.16micron filter. We have observed 3 square arcminute…
Review: Understanding Galaxy Formation and Evolution with Long Wavelength Observations
Matthew A. Malkan
It is well established in the local Universe that regions of high star-formation rate are dusty. As a result of this physical causal link, galaxies of increasing current star forma…
The U.S. ISO Key Project on Quasars
Eric Hooper, Belinda Wilkes, Kim McLeod +5
Observations for the U.S. key project on quasars using ISO were completed in April when the satellite's cryogen supply expired. This proceeding presents an update of the project, i…
The Disks of Galaxies with Seyfert and Starburst Nuclei: II. Near-Infrared Structural Properties
L. K. Hunt, M. A. Malkan, G. Moriondo +1
We have derived the near-infrared structural components of a sample of Seyfert and starburst (SBN) host galaxies by fitting the images of Hunt et al. (1997,ApJS,108,229) with a new…
Steps towards determination of the size and structure of the Broad-Line Region in Active Galactic Nuclei. XIII. Ultraviolet observations of the Broad-Line Radio Galaxy 3C 390.3
The International AGN Watch, :, P. T. O'Brien +15
As part of an extensive multi-wavelength monitoring campaign, the International Ultraviolet Explorer satellite was used to observe the broad-line radio galaxy 3C 390.3 during the p…