Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/32966
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | UMANA, Grazia Maria Gloria | en_US |
dc.contributor.author | BUEMI, CARLA SIMONA | en_US |
dc.contributor.author | TRIGILIO, CORRADO | en_US |
dc.contributor.author | LETO, PAOLO | en_US |
dc.contributor.author | Hora, Joseph L. | en_US |
dc.contributor.author | Fazio, Giovanni | en_US |
dc.date.accessioned | 2023-01-20T15:59:02Z | - |
dc.date.available | 2023-01-20T15:59:02Z | - |
dc.date.issued | 2011 | en_US |
dc.identifier.issn | 0037-9565 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/32966 | - |
dc.description.abstract | We present first results of our study of a sample of Galactic LBV, aimed to contribute to a better understanding of the LBV phenomenon, by recovering the mass-loss history of the central object from the analysis of its associated nebula. Mass-loss properties have been derived by a synergistic use of different techniques, at different wavelengths, to obtain high-resolution, multi-wavelength maps, tracing the different emitting components coexisting in the stellar ejecta: the ionized/neutral gas and the dust. Evidence for asymmetric mass-loss and observational evidence of possible mutual interaction between gas and dust components have been observed by the comparison of mid-IR (Spitzer/IRAC, VLT/VISIR) and radio (VLA) images of the nebulae, while important information on the gas and dust composition have been derived from Spitzer/IRS spectra. | en_US |
dc.language.iso | eng | en_US |
dc.title | The nebulae around LBVs: a multiwavelength approach | en_US |
dc.type | Article | - |
dc.identifier.url | https://popups.uliege.be/0037-9565/index.php?id=2785 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 80 | en_US |
dc.relation.firstpage | 335 | en_US |
dc.relation.lastpage | 340 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 6 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | BULLETIN DE LA SOCIÉTÉ ROYALE DES SCIENCES DE LIÈGE | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2011BSRSL..80..335U | 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.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 0037-9565 | - |
crisitem.journal.ance | E027087 | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.orcid | 0000-0002-6972-8388 | - |
crisitem.author.orcid | 0000-0002-7288-4613 | - |
crisitem.author.orcid | 0000-0002-1216-7831 | - |
crisitem.author.orcid | 0000-0003-4864-2806 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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document.pdf | PDF editoriale | 333.52 kB | Adobe PDF | Visualizza/apri |
1011.3730.pdf | arXiv | 285.69 kB | Adobe PDF | Visualizza/apri |
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