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CO in infrared luminous galaxies

Name: CO in infrared luminous galaxies
Keywords: Starburst Galaxy, High Luminosity, Star Formation, Bright Galaxy, 500, 520, Spiral Galaxy

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 06 Apr 2008 United States Publisher:Springer Berlin Heidelberg

Authors: Sanders, D. B.; Soifer, B. T.; Scoville, N. Z.;

doi: 10.1007/3-540-50438-9_302

CO in infrared luminous galaxies

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Abstract

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 LâŠ™ (H_o = 75 km s^(-1)Mpc^(-1)) exceeding that of Seyfert galaxies and quasars (Soifer et al. 1986). ; Â© 1988 Springer-Verlag.

Country

United States

Related Organizations

California Institute of Technology
United States

Keywords

Starburst Galaxy, High Luminosity, Star Formation, Bright Galaxy, 500, 520, Spiral Galaxy

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