Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/34319
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Liu, K. | en_US |
dc.contributor.author | Antoniadis, J. | en_US |
dc.contributor.author | Bassa, C. G. | en_US |
dc.contributor.author | Chen, S. | en_US |
dc.contributor.author | Cognard, I. | en_US |
dc.contributor.author | Gaikwad, M. | en_US |
dc.contributor.author | Hu, H. | en_US |
dc.contributor.author | Jang, J. | en_US |
dc.contributor.author | Janssen, G. H. | en_US |
dc.contributor.author | Karuppusamy, R. | en_US |
dc.contributor.author | Kramer, M. | en_US |
dc.contributor.author | Lee, K. J. | en_US |
dc.contributor.author | Main, R. A. | en_US |
dc.contributor.author | Mall, G. | en_US |
dc.contributor.author | McKee, J. W. | en_US |
dc.contributor.author | Mickaliger, M. B. | en_US |
dc.contributor.author | PERRODIN, DELPHINE | en_US |
dc.contributor.author | Sanidas, S. A. | en_US |
dc.contributor.author | Stappers, B. W. | en_US |
dc.contributor.author | Wang, L. | en_US |
dc.contributor.author | Zhu, W. W. | en_US |
dc.contributor.author | BURGAY, MARTA | en_US |
dc.contributor.author | CONCU, Raimondo | en_US |
dc.contributor.author | CORONGIU, ALESSANDRO | en_US |
dc.contributor.author | MELIS, Andrea | en_US |
dc.contributor.author | PILIA, Maura | en_US |
dc.contributor.author | POSSENTI, ANDREA | en_US |
dc.date.accessioned | 2023-07-21T15:15:19Z | - |
dc.date.available | 2023-07-21T15:15:19Z | - |
dc.date.issued | 2022 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/34319 | - |
dc.description.abstract | We report on the detection of quasi-periodic micro-structure in three millisecond pulsars (MSPs), PSRs J1022+1001, J2145-0750 and J1744-1134, using high time resolution data acquired with the Large European Array for Pulsars at a radio frequency of 1.4 GHz. The occurrence rate of quasi-periodic micro-structure is consistent among pulses with different peak flux densities. Using an auto-correlation analysis, we measure the periodicity and width of the micro-structure in these three pulsars. The detected micro-structure from PSRs J1022+1001 and J1744-1134 is often highly linearly polarised. In PSR J1022+1001, the linear polarisation position angles of micro-structure pulses are in general flat with a small degree of variation. Using these results, we further examine the frequency and rotational period dependency of micro-structure properties established in previous work, along with the angular beaming and temporal modulation models that explains the appearance of micro-structure. We also discuss a possible link of micro-structure to the properties of some of the recently discovered fast radio bursts which exhibit a very similar emission morphology. | en_US |
dc.language.iso | eng | en_US |
dc.title | Detection of quasi-periodic micro-structure in three millisecond pulsars with the Large European Array for Pulsars | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stac1082 | en_US |
dc.identifier.scopus | 2-s2.0-85133094795 | en_US |
dc.identifier.url | http://arxiv.org/abs/2206.10045v1 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/513/3/4037/6575043 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 513 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 4037 | en_US |
dc.relation.lastpage | 4044 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 27 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | GBR | en_US |
dc.contributor.country | FRA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | CAN | en_US |
dc.contributor.country | GRC | en_US |
dc.contributor.country | NLD | en_US |
dc.contributor.country | CHN | 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.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 | Article | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0002-1806-2483 | - |
crisitem.author.orcid | 0000-0002-8265-4344 | - |
crisitem.author.orcid | 0000-0003-3621-349X | - |
crisitem.author.orcid | 0000-0002-5924-3141 | - |
crisitem.author.orcid | 0000-0002-6558-1315 | - |
crisitem.author.orcid | 0000-0001-7397-8091 | - |
crisitem.author.orcid | 0000-0001-5902-3731 | - |
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