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

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.

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 Creators:
Dasyra, K. M.1, Author           
Xilouris, E. M., Author
Misiriotis, A., Author
Kylafis, N. D., Author
Affiliations:
1Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159889              

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Language(s): eng - English
 Dates: 2005
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Internal
 Identifiers: eDoc: 230178
Other: AS 20/67, p.197-200
 Degree: -

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Title: The spectral energy Distributions of gas-rich Galaxies: Confronting Models with Data
Place of Event: Heidelberg, Germany
Start-/End Date: 2004-10-04 - 2004-10-08

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Title: The spectral energy Distributions of gas-rich Galaxies: Confronting Models with Data
Source Genre: Proceedings
 Creator(s):
Popescu, Cristina C., Editor
Tuffs, Richard J., Editor
Affiliations:
-
Publ. Info: Melville, New York : American Institute of Physics
Pages: 465 Volume / Issue: - Sequence Number: - Start / End Page: 197 - 200 Identifier: ISBN: 0-7354-0246-9

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Title: AIP Conference Proceedings
Source Genre: Series
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Publ. Info: -
Pages: - Volume / Issue: 761 Sequence Number: - Start / End Page: - Identifier: ISSN: 0094-243X