Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27761
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Cameron, A. D. | en_US |
dc.contributor.author | Champion, D. J. | en_US |
dc.contributor.author | Kramer, M. | en_US |
dc.contributor.author | Bailes, M. | en_US |
dc.contributor.author | Barr, E. D. | en_US |
dc.contributor.author | Bassa, C. G. | en_US |
dc.contributor.author | Bhandari, S. | en_US |
dc.contributor.author | Bhat, N. D. R. | en_US |
dc.contributor.author | BURGAY, MARTA | en_US |
dc.contributor.author | Burke-Spolaor, S. | en_US |
dc.contributor.author | Eatough, R. P. | en_US |
dc.contributor.author | Flynn, C. M. L. | en_US |
dc.contributor.author | Freire, P. C. C. | en_US |
dc.contributor.author | Jameson, A. | en_US |
dc.contributor.author | Johnston, S. | en_US |
dc.contributor.author | Karuppusamy, R. | en_US |
dc.contributor.author | Keith, M. J. | en_US |
dc.contributor.author | Levin, L. | en_US |
dc.contributor.author | Lorimer, D. R. | en_US |
dc.contributor.author | Lyne, A. G. | en_US |
dc.contributor.author | McLaughlin, M. A. | en_US |
dc.contributor.author | Ng, C. | en_US |
dc.contributor.author | Petroff, E. | en_US |
dc.contributor.author | POSSENTI, ANDREA | en_US |
dc.contributor.author | RIDOLFI, ALESSANDRO | en_US |
dc.contributor.author | Stappers, B. W. | en_US |
dc.contributor.author | van Straten, W. | en_US |
dc.contributor.author | Tauris, T. M. | en_US |
dc.contributor.author | Tiburzi, C. | en_US |
dc.contributor.author | Wex, N. | en_US |
dc.date.accessioned | 2020-10-13T13:26:41Z | - |
dc.date.available | 2020-10-13T13:26:41Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27761 | - |
dc.description.abstract | We report the discovery of PSR J1757-1854, a 21.5-ms pulsar in a highly-eccentric, 4.4-h orbit with a neutron star (NS) companion. PSR J1757-1854 exhibits some of the most extreme relativistic parameters of any known pulsar, including the strongest relativistic effects due to gravitational-wave damping, with a merger time of 76 Myr. Following a 1.6-yr timing campaign, we have measured five post-Keplerian parameters, yielding the two component masses (m<SUB>p</SUB> = 1.3384(9) M<SUB>☉</SUB> and m<SUB>c</SUB> = 1.3946(9) M<SUB>☉</SUB>) plus three tests of general relativity, which the theory passes. The larger mass of the NS companion provides important clues regarding the binary formation of PSR J1757-1854. With simulations suggesting 3-σ measurements of both the contribution of Lense-Thirring precession to the rate of change of the semimajor axis and the relativistic deformation of the orbit within ∼7-9 yr, PSR J1757-1854 stands out as a unique laboratory for new tests of gravitational theories. | en_US |
dc.language.iso | eng | en_US |
dc.title | The High Time Resolution Universe Pulsar Survey - XIII. PSR J1757-1854, the most accelerated binary pulsar | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnrasl/sly003 | en_US |
dc.identifier.scopus | 2-s2.0-85060844180 | en_US |
dc.identifier.isi | 000438222600013 | en_US |
dc.identifier.url | https://academic.oup.com/mnrasl/article-abstract/475/1/L57/4794951 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 475 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | L57 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018MNRAS.475L..57C | 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 | 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. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0002-8265-4344 | - |
crisitem.author.orcid | 0000-0001-5902-3731 | - |
crisitem.author.orcid | 0000-0001-6762-2638 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
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File | Description | Size | Format | |
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Cameron2018.pdf | Pdf editoriale | 288.52 kB | Adobe PDF | View/Open |
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