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Modelling the dust content of spiral galaxies: more dust mass vs. enhanced dust grain emissivity

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Dasyra,  K. M.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Dasyra, K. M., Xilouris, E. M., Misiriotis, A., & Kylafis, N. D. (2005). Modelling the dust content of spiral galaxies: more dust mass vs. enhanced dust grain emissivity. In C. C. Popescu, & R. J. Tuffs (Eds.), The spectral energy Distributions of gas-rich Galaxies: Confronting Models with Data (pp. 197-200). Melville, New York: American Institute of Physics.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-DC02-4
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