Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27026
DC Field | Value | Language |
---|---|---|
dc.contributor.author | SIDOLI, Lara | en_US |
dc.date.accessioned | 2020-09-01T10:14:49Z | - |
dc.date.available | 2020-09-01T10:14:49Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 1824-8039 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27026 | - |
dc.description.abstract | I present a brief up-to-date review of the current understanding of Supergiant Fast X-ray Transients, with an emphasis on the observational point of view. After more than a decade since their discovery, a remarkable progress has been made in getting the picture of their phenomenology at X-ray energies. However, a similar in-depth investigation of the properties of the supergiant companions is needed, but has started more recently. A multifrequency approach is the key to fully understand the physical mechanism driving the SFXT behaviour, still under debate. | en_US |
dc.language.iso | eng | en_US |
dc.title | Supergiant Fast X-ray Transients - A short review | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.22323/1.306.0052 | en_US |
dc.identifier.url | https://pos.sissa.it/306/052 | en_US |
dc.identifier.url | https://arxiv.org/pdf/1710.03943.pdf | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 306 | en_US |
dc.relation.firstpage | 52 | en_US |
dc.relation.lastpage | 65 | en_US |
dc.relation.numberofpages | 14 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 1 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.alleditors | Giovannelli F.; Sabau-Graziati, L. | en_US |
dc.relation.ispartofbook | XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop (MULTIF2017) | en_US |
dc.type.invited | sì | en_US |
dc.relation.conferencename | XII Multifrequency Behaviour of High Energy Cosmic Sources Workshop | en_US |
dc.relation.conferenceplace | Palermo | en_US |
dc.relation.conferencedate | 12-17 giugno, 2017 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | POS PROCEEDINGS OF SCIENCE | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2017mbhe.confE..52S | 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 | Conference paper | - |
crisitem.journal.journalissn | 1824-8039 | - |
crisitem.journal.ance | E188909 | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0001-9705-2883 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
sidoli2017_sfxt_MULTIF2017_052.pdf | PDF editoriale | 684.63 kB | Adobe PDF | View/Open |
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