Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29499
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Safi-Harb, Samar | en_US |
dc.contributor.author | AMATO, Elena | en_US |
dc.contributor.author | Gotthelf, Eric V. | en_US |
dc.contributor.author | Katsuda, Satoru | en_US |
dc.contributor.author | Sasaki, Manami | en_US |
dc.contributor.author | Uchiyama, Yasunobu | en_US |
dc.contributor.author | Tsuji, Naomi | en_US |
dc.contributor.author | Guest, Benson | en_US |
dc.date.accessioned | 2021-01-05T16:20:59Z | - |
dc.date.available | 2021-01-05T16:20:59Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 2330-9458 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29499 | - |
dc.description.abstract | Supernova remnants and neutron stars serve as nearby laboratories relevant to many areas in Astrophysics. In this white paper, we highlight some science breakthroughs to be achieved with future X-ray missions (such as the proposed AXIS probe) equipped with sub-arcsecond imaging resolution and an order of magnitude improvement in sensitivity. | en_US |
dc.language.iso | eng | en_US |
dc.title | High-Resolution X-ray Imaging Studies of Neutron Stars, Pulsar Wind Nebulae and Supernova Remnants | en_US |
dc.type | Article | - |
dc.identifier.url | https://baas.aas.org/pub/2020n3i317/release/1 | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.volume | 51 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 317 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.numberofauthors | 8 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | USA | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | BULLETIN OF THE AMERICAN ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019BAAS...51c.317S | 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 | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0002-9881-8112 | - |
crisitem.journal.journalissn | 2330-9458 | - |
crisitem.journal.ance | E224837 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
19WhitePaper.pdf | postprint | 925.56 kB | Adobe PDF | View/Open |
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