Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30005
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Munar-Adrover, Pere | en_US |
dc.contributor.author | PIANO, Giovanni | en_US |
dc.contributor.author | Sabatini, S. | en_US |
dc.contributor.author | TAVANI, MARCO | en_US |
dc.contributor.author | LUCARELLI, Fabrizio | en_US |
dc.contributor.author | VERRECCHIA, Francesco | en_US |
dc.contributor.author | PITTORI, Carlotta | en_US |
dc.date.accessioned | 2021-01-26T13:26:11Z | - |
dc.date.available | 2021-01-26T13:26:11Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.isbn | 978-0-7354-1456-3 | en_US |
dc.identifier.issn | 0094-243X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30005 | - |
dc.description.abstract | The AGILE satellite has been proven to be an excellent tool to study transient gamma-ray sources since it entered in a spinning operational mode in 2009. Thanks to its scanning capabilities it observes the whole sky every few hours. Several new interesting systems were discovered, such as AGL J2241+4454 in 2010, probably associated to the mysterious black-hole high-mass X-ray binary MWC 656. With a state of the art PSF and sensitivity in the 100 MeV – 1 GeV energy range, AGILE studied this system in order to identify new periods of gamma-ray activity that could be associated to the binary, and found a total of 10 flares spanning from 2008 until 2013. AGILE studied also the Cygnus region, finding evidence of a new recent gamma-ray flare from the microquasar Cygnus X-3, with a flux of ∼ 2×10−8 ph cm−2 s, during a state transition phase in the bright high-soft X-ray state. Also Cygnus X-1 was detected in the past by AGILE, although both systems are very different and show different behaviour. | en_US |
dc.language.iso | eng | en_US |
dc.title | Galactic microquasar transients with AGILE | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1063/1.4968919 | en_US |
dc.identifier.scopus | 2-s2.0-85010931178 | en_US |
dc.identifier.isi | 000399207800034 | en_US |
dc.identifier.url | https://aip.scitation.org/doi/abs/10.1063/1.4968919 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 1792 | en_US |
dc.relation.issue | 1 | en |
dc.relation.firstpage | 040015 | en_US |
dc.type.referee | REF_0 | en_US |
dc.relation.alleditors | Aharonian, Felix A.; Hofmann, Werner; Rieger, Frank M. | en_US |
dc.relation.ispartofbook | 6th International Symposium on High Energy Gamma-Ray Astronomy | en_US |
dc.relation.conferencename | 6th International Symposium on High Energy Gamma-Ray Astronomy | en_US |
dc.relation.conferenceplace | Heidelberg, Germany | en_US |
dc.relation.conferencedate | 11–15 July, 2016 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | AIP CONFERENCE PROCEEDINGS | en_US |
dc.identifier.adsbibcode | 2017AIPC.1792d0015M | 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 | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.orcid | 0000-0002-9332-5319 | - |
crisitem.author.orcid | 0000-0003-2893-1459 | - |
crisitem.author.orcid | 0000-0002-6311-764X | - |
crisitem.author.orcid | 0000-0003-3455-5082 | - |
crisitem.author.orcid | 0000-0001-6661-9779 | - |
crisitem.journal.journalissn | 0094-243X | - |
crisitem.journal.ance | E211233 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
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Munar 2017 AIPC 1792 040015.pdf | Pdf editoriale | 554.9 kB | Adobe PDF | View/Open |
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