|Author||Thronson, H. A. (Jr.) ♦ Hunter, D. A. ♦ Casey, S. ♦ Harper, D. A. ♦ Latter, W. B.|
|Source||United States Department of Energy Office of Scientific and Technical Information|
|Subject Keyword||CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ♦ GALAXIES ♦ GRAVITATIONAL INTERACTIONS ♦ COSMIC DUST ♦ EMISSION SPECTRA ♦ ENERGY SPECTRA ♦ INFRARED SPECTRA ♦ INTERSTELLAR SPACE ♦ SPECTROSCOPY ♦ STAR EVOLUTION ♦ VISIBLE SPECTRA ♦ BASIC INTERACTIONS ♦ DUSTS ♦ INTERACTIONS ♦ SPACE ♦ SPECTRA ♦ Astrophysics & Cosmology- Galaxies|
|Abstract||The 100- and 160-micron continuum emission from cool dust in the interacting gas-rich pair of galaxies, NGC 4490 and NGC 4485, was mapped. Visual continuum and H-alpha images of the pair were obtained. The state of the interstellar medium and the rate and efficiency of star formation are investigated. 49 refs.|
|Learning Resource Type||Article|
|Publisher Department||Wyoming Infrared Observatory, Laramie (USA) ♦ Lowell Observatory, Flagstaff, AZ (USA) ♦ Yerkes Observatory, Williams Bay, WI (USA) ♦ Steward Observatory, Tucson, AZ (USA)|
|Publisher Place||United States|
|Organization||Wyoming Infrared Observatory, Laramie (USA) ♦ Lowell Observatory, Flagstaff, AZ (USA) ♦ Yerkes Observatory, Williams Bay, WI (USA) ♦ Steward Observatory, Tucson, AZ (USA)|
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