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arXiv · 0912.3032

MOIRCS Deep Survey V: A Universal Relation for Stellar Mass and Surface Brightness of Galaxies

Takashi Ichikawa·Masaru Kajisawa·Toru Yamada·Masayuki Akiyama·Tomohiro Yoshikawa·Masato Onodera·Masahiro Konishi
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Abstract

We present a universal linear correlation between the stellar mass and surface brightness (SB) of galaxies at 0.3 0) and the massive galaxies (M_*>10^(10)M_sun) shows stronger brightening, (1+z)^(-1.5+-0.1). Based on the comparison with galaxy evolution models, we find that the phenomena are well explained by the pure luminosity evolution of galaxies out to z~3.

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Takashi Ichikawa, Masaru Kajisawa, Toru Yamada, Masayuki Akiyama, Tomohiro Yoshikawa, Masato Onodera, Masahiro Konishi. 2009-12-15. MOIRCS Deep Survey V: A Universal Relation for Stellar Mass and Surface Brightness of Galaxies. https://doi.org/10.1088/0004-637x%2F709%2F2%2F741

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