Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26052
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Kino, M. | en_US |
dc.contributor.author | Ito, H. | en_US |
dc.contributor.author | Kawakatu, N. | en_US |
dc.contributor.author | ORIENTI, Monica | en_US |
dc.contributor.author | Nagai, H. | en_US |
dc.contributor.author | Wajima, K. | en_US |
dc.contributor.author | Itoh, R. | en_US |
dc.date.accessioned | 2020-06-15T10:20:34Z | - |
dc.date.available | 2020-06-15T10:20:34Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0004-6337 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26052 | - |
dc.description.abstract | We investigate shell emission associated with dying radio loud AGNs. First, based on our recent work by Ito et al. (2015), we describe the dynamical and spectral evolution of shells after stopping the jet energy injection. We find that the shell emission overwhelms that of the radio lobes soon after stopping the jet energy injection because fresh electrons are continuously supplied into the shell via the forward shock, while the radio lobes rapidly fade out without jet energy injection. We find that such fossil shells can be a new class of target sources for SKA telescope. Next, we apply the model to the nearby radio source 3C84. Then, we find that the fossil shell emission in 3C84 is less luminous in the radio band while it is bright in the TeV γ-ray band and can be detectable by CTA. Data from STELLA | en_US |
dc.language.iso | eng | en_US |
dc.title | Fossil shell emission in dying radio loud AGNs | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1002/asna.201512263 | en_US |
dc.identifier.scopus | 2-s2.0-84959010457 | en_US |
dc.identifier.isi | 000370147600007 | en_US |
dc.identifier.url | http://arxiv.org/abs/1511.03090v1 | en_US |
dc.identifier.url | https://onlinelibrary.wiley.com/doi/abs/10.1002/asna.201512263 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 337 | en_US |
dc.relation.firstpage | 47 | en_US |
dc.relation.lastpage | 51 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMISCHE NACHRICHTEN | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016AN....337...47K | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | 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.cerifentitytype | Publications | - |
item.openairetype | Article | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
crisitem.journal.journalissn | 0004-6337 | - |
crisitem.journal.ance | E016235 | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0003-4470-7094 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
kino-css.pdf | postprint | 423.21 kB | Adobe PDF | View/Open |
asna.201512263.pdf | [Administrators only] | 325.95 kB | Adobe PDF |
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