1. Color-size Relations of Disk Galaxies with Equivalent Masses
- Author
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Zhang Bo, Fu Wei, Chang Rui-xiang, and Shen Shi-yin
- Subjects
Physics ,Luminous infrared galaxy ,Astronomy ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Galaxy merger ,Peculiar galaxy ,Space and Planetary Science ,Galaxy group ,Thick disk ,Elliptical galaxy ,Astrophysics::Earth and Planetary Astrophysics ,Disc ,Lenticular galaxy ,Astrophysics::Galaxy Astrophysics - Abstract
The local face-on disk galaxies are selected as galaxy sample from the main galaxy sample of the Seventh Data Release of Sloan Digital Sky Survey (SDSS DR7). The correlations between the colors and sizes of disk galaxies with equivalent total stellar masses are statistically investigated and their realities are tested. It is found that for the disk galaxies with equivalent masses, the correlation between u-r color and size is very weak. However, there are anticorrelations between g-r, r-i, r-z colors and sizes, i.e., the larger are the sizes of galaxies, the bluer are their colors. This result means that the mass distribution of disk galaxies has a significant influence on their star formation history. The galaxies with more extended mass distributions evolve more slowly.
- Published
- 2011