Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29039
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Chernyakova, M. | en_US |
dc.contributor.author | Malyshev, D. | en_US |
dc.contributor.author | PAIZIS, ADAMANTIA | en_US |
dc.contributor.author | LA PALOMBARA, NICOLA | en_US |
dc.contributor.author | Balbo, M. | en_US |
dc.contributor.author | Walter, R. | en_US |
dc.contributor.author | Hnatyk, B. | en_US |
dc.contributor.author | van Soelen, B. | en_US |
dc.contributor.author | ROMANO, Patrizia | en_US |
dc.contributor.author | Munar-Adrover, P. | en_US |
dc.contributor.author | Vovk, Ie. | en_US |
dc.contributor.author | PIANO, Giovanni | en_US |
dc.contributor.author | CAPITANIO, FIAMMA | en_US |
dc.contributor.author | Falceta-Gonçalves, D. | en_US |
dc.contributor.author | LANDONI, Marco | en_US |
dc.contributor.author | Luque-Escamilla, P. L. | en_US |
dc.contributor.author | Martí, J. | en_US |
dc.contributor.author | Paredes, J. M. | en_US |
dc.contributor.author | Ribó, M. | en_US |
dc.contributor.author | Safi-Harb, S. | en_US |
dc.contributor.author | Saha, L. | en_US |
dc.contributor.author | SIDOLI, Lara | en_US |
dc.contributor.author | VERCELLONE, STEFANO | en_US |
dc.date.accessioned | 2020-12-21T10:43:46Z | - |
dc.date.available | 2020-12-21T10:43:46Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0004-6361 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29039 | - |
dc.description.abstract | Aims: Despite recent progress in the field, there are still many open questions regarding γ-ray binaries. In this paper we provide an overview of non-transient γ-ray binaries and discuss how observations with the Cherenkov Telescope Array (CTA) will contribute to their study. Methods: We simulated the spectral behaviour of the non-transient γ-ray binaries using archival observations as a reference. With this we tested the CTA capability to measure the spectral parameters of the sources and detect variability on various timescales. <BR /> Results: We review the known properties of γ-ray binaries and the theoretical models that have been used to describe their spectral and timing characteristics. We show that the CTA is capable of studying these sources on timescales comparable to their characteristic variability timescales. For most of the binaries, the unprecedented sensitivity of the CTA will allow studying the spectral evolution on a timescale as short as 30 min. This will enable a direct comparison of the TeV and lower energy (radio to GeV) properties of these sources from simultaneous observations. We also review the source-specific questions that can be addressed with these high-accuracy CTA measurements. | en_US |
dc.language.iso | eng | en_US |
dc.title | Overview of non-transient γ-ray binaries and prospects for the Cherenkov Telescope Array | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1051/0004-6361/201936501 | en_US |
dc.identifier.scopus | 2-s2.0-85075883971 | en_US |
dc.identifier.isi | 000515103800002 | en_US |
dc.identifier.url | https://www.aanda.org/articles/aa/abs/2019/11/aa36501-19/aa36501-19.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 631 | en_US |
dc.relation.firstpage | A177 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 23 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | ESP | en_US |
dc.contributor.country | BRA | en_US |
dc.contributor.country | CAN | en_US |
dc.contributor.country | IRL | en_US |
dc.contributor.country | CHE | en_US |
dc.contributor.country | UKR | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMY & ASTROPHYSICS | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019A&A...631A.177C | 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::PE9_10 High energy and particle astronomy – X-rays, cosmic rays, gamma rays, neutrinos | 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.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0001-5067-0377 | - |
crisitem.author.orcid | 0000-0001-7015-6359 | - |
crisitem.author.orcid | 0000-0003-0258-7469 | - |
crisitem.author.orcid | 0000-0002-9332-5319 | - |
crisitem.author.orcid | 0000-0002-6384-3027 | - |
crisitem.author.orcid | 0000-0001-5570-5081 | - |
crisitem.author.orcid | 0000-0001-9705-2883 | - |
crisitem.author.orcid | 0000-0003-1163-1396 | - |
crisitem.journal.journalissn | 0004-6361 | - |
crisitem.journal.ance | E016240 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1909.11018.pdf | postprint | 960.6 kB | Adobe PDF | View/Open |
aa36501-19.pdf | Pdf editoriale | 1.27 MB | Adobe PDF | View/Open |
Page view(s)
57
checked on Mar 29, 2024
Download(s)
45
checked on Mar 29, 2024
Google ScholarTM
Check
Altmetric
Altmetric
Items in DSpace are published in Open Access, unless otherwise indicated.