Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/33066
DC Field | Value | Language |
---|---|---|
dc.contributor.author | BIANCHI, Simone | en_US |
dc.date.accessioned | 2023-01-26T09:59:42Z | - |
dc.date.available | 2023-01-26T09:59:42Z | - |
dc.date.issued | 2005 | en_US |
dc.identifier.isbn | 0735402469 | en_US |
dc.identifier.issn | 0094-243X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/33066 | - |
dc.description.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. | en_US |
dc.language.iso | eng | en_US |
dc.title | Radiative Transfer in Spiral Galaxies: Dust Extinction and Emission | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1063/1.1913928 | en_US |
dc.identifier.scopus | 2-s2.0-33748568098 | en_US |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/33748568098 | en_US |
dc.identifier.url | https://aip.scitation.org/doi/pdf/10.1063/1.1913928 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 761 | en_US |
dc.relation.firstpage | 178 | en_US |
dc.relation.lastpage | 186 | en_US |
dc.type.referee | REF_0 | en_US |
dc.relation.alleditors | Popescu, Cristina C.; Tuffs, Richard J. | en_US |
dc.relation.ispartofbook | The spectral energy distribution of gas-rich galaxies: confronting models with data | en_US |
dc.publisher.name | American Institute of Physics, 1970- | en_US |
dc.type.invited | sì | en_US |
dc.relation.conferencename | THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop | en_US |
dc.relation.conferenceplace | Heidelberg, Germany | en_US |
dc.relation.conferencedate | October 4-8, 2004 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | AIP CONFERENCE PROCEEDINGS | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2005AIPC..761..178B | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.fulltext | With Fulltext | - |
item.openairetype | Conference paper | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0094-243X | - |
crisitem.journal.ance | E211233 | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0002-9384-846X | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
03-BianchiProc2005.pdf | postprint | 167.3 kB | Adobe PDF | View/Open |
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