CO in infrared luminous galaxies
CO in infrared luminous galaxies
There has been considerable recent interest in the properties of infrared galaxies due to the discovery by the Infrared Astronomical Satellite (IRAS) of a class of luminous galaxies which emit the bulk of their energy in the far-infrared (Houck et al. 1984; Soifer et al. 1984). Ground-based studies of these infrared luminous galaxies have shown that they are a substantial component of the local universe (z ~ 0.1) with a space density at luminosities above 1011 L⊙ (H_o = 75 km s^(-1)Mpc^(-1)) exceeding that of Seyfert galaxies and quasars (Soifer et al. 1986). ; © 1988 Springer-Verlag.
- California Institute of Technology United States
Starburst Galaxy, High Luminosity, Star Formation, Bright Galaxy, 500, 520, Spiral Galaxy
Starburst Galaxy, High Luminosity, Star Formation, Bright Galaxy, 500, 520, Spiral Galaxy
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