Galaxy clustering as a function of surface brightness
نویسندگان
چکیده
منابع مشابه
158 μ m brightness as a function of galaxy activity
We investigate the possibility that the known decrease in the relative luminosity of the 158 μm [C II] line with the far-infrared luminosity in extragalactic sources is due to evolutionary effects: Because of the flux limited nature of the surveys, large luminosities are indicative of large distances, and we do find significant increases in both L[CII] and LFIR with redshift. However, the fact ...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 1985
ISSN: 0004-637X,1538-4357
DOI: 10.1086/163678