The nature of the red disk-like galaxies at high redshift: dust attenuation vs. 
intrinsically red stellar populations

Pierini, D.; Maraston, C.; Gordon, K. D.; Witt, A. N.

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The nature of the red disk-like galaxies at high redshift: dust attenuation vs. intrinsically red stellar populations

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Pierini, D.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Maraston, C.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Pierini, D., Maraston, C., Gordon, K. D., & Witt, A. N. (2005). The nature of the red disk-like galaxies at high redshift: dust attenuation vs. intrinsically red stellar populations. In C. C. Popescu, & R. J. Tuffs (Eds.), The spectral energy Distributions of gas-rich Galaxies: Confronting Models with Data (pp. 313-319). Melville, New York: American Institute of Physics.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-DC05-D

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