Abstract
It has been demonstrated that galaxy populations vary with the density of neighboring galaxies (Dressier, 1980) or the radius from the center of a galaxy cluster (Whitmore et al., 1993). The increase in the fraction of blue, star-forming cluster galaxies with redshift (Butcher & Oemler, 1978) has been well established as well. However, the physical mechanisms responsible for these effects are not fully understood yet.
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References
Butcher, H., & Oemler, A. Jr. 1978, ApJ, 301, 57.
Dressier, A. 1980, ApJ, 236, 351.
Whitmore, B.C., Gilmore, D.M., & Jones, C. 1993, ApJ, 407, 489.
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© 1999 Springer Science+Business Media Dordrecht
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Okamoto, T., Habe, A. (1999). Formation and Evolution of Galactic Halos in Clusters of Galaxies. In: Miyama, S.M., Tomisaka, K., Hanawa, T. (eds) Numerical Astrophysics. Astrophysics and Space Science Library, vol 240. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4780-4_16
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DOI: https://doi.org/10.1007/978-94-011-4780-4_16
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