Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28604
DC Field | Value | Language |
---|---|---|
dc.contributor.author | DE LUCA, Andrea | en_US |
dc.date.accessioned | 2020-12-01T15:38:05Z | - |
dc.date.available | 2020-12-01T15:38:05Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 1742-6588 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28604 | - |
dc.description.abstract | Central Compact Objects (CCOs) are a handful of sources located close to the geometrical center of young supernova remnants. They only show thermal-like, soft X-ray emission and have no counterparts at any other wavelength. While the first observed CCO turned out to be a very peculiar magnetar, discovery that three members of the family are weakly magnetised Isolated Neutron Stars (INSs) set the basis for an interpretation of the class. However, the phenomeology of CCOs and their relationship with other classes of INSs, possibly ruled by supernova fall-back accretion, are still far from being well understood. | en_US |
dc.language.iso | eng | en_US |
dc.title | Central compact objects in supernova remnants | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1088/1742-6596/932/1/012006 | en_US |
dc.identifier.scopus | 2-s2.0-85039415489 | en_US |
dc.identifier.isi | 000426770000006 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.1088/1742-6596/932/1/012006 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 932 | en_US |
dc.relation.issue | 1 | en |
dc.relation.firstpage | 012006 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 1 | en_US |
dc.description.international | no | en_US |
dc.relation.ispartofbook | International Conference Physics of Neutron Stars - 2017. 50 years after. 10–14 July 2017 | en_US |
dc.type.invited | sì | en_US |
dc.relation.conferencename | International Conference Physics of Neutron Stars - 2017. 50 years after. 10–14 July 2017 | en_US |
dc.relation.conferenceplace | Saint Petersburg, Russia | en_US |
dc.relation.conferencedate | 10-14 July, 2017 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | JOURNAL OF PHYSICS. CONFERENCE SERIES | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.identifier.adsbibcode | 2017JPhCS.932a2006D | 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.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Conference paper | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 1742-6588 | - |
crisitem.journal.ance | E187130 | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0001-6739-687X | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
De_Luca_2017_J._Phys.__Conf._Ser._932_012006.pdf | Pdf editoriale | 520.24 kB | Adobe PDF | View/Open |
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