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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 3 CONTRIBUTI IN ATTI DI CONVEGNO (Proceedings)
  4. 3.01 Contributi in Atti di convegno
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/33066
Title: Radiative Transfer in Spiral Galaxies: Dust Extinction and Emission
Authors: BIANCHI, Simone 
Issue Date: 2005
Journal: AIP CONFERENCE PROCEEDINGS 
Volume: The spectral energy distribution of gas-rich galaxies: confronting models with data
Editors: Popescu, Cristina C.; Tuffs, Richard J.
Number: 761
First Page: 178
Abstract: I review the results of our Monte Carlo models for the radiative transfer in the dusty disks of spiral galaxies. The simulations are compared to observations of dust extinction in the optical and emission in the FIR, with the aim of deriving the amount of interstellar grains, their distribution and the internal extinction in a galaxy. I discuss the main, puzzling, result of this comparison: more dust is needed to explain thermal emission than what is inferred from extinction studies.
Conference Name: THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop
Conference Place: Heidelberg, Germany
Conference Date: October 4-8, 2004
URI: http://hdl.handle.net/20.500.12386/33066
URL: https://api.elsevier.com/content/abstract/scopus_id/33748568098
https://aip.scitation.org/doi/pdf/10.1063/1.1913928
ISSN: 0094-243X
ISBN: 0735402469
DOI: 10.1063/1.1913928
Bibcode ADS: 2005AIPC..761..178B
Fulltext: open
Appears in Collections:3.01 Contributi in Atti di convegno

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