Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30880
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Freire, P. C. C. | en_US |
dc.contributor.author | RIDOLFI, ALESSANDRO | en_US |
dc.contributor.author | Kramer, M. | en_US |
dc.contributor.author | Jordan, C. | en_US |
dc.contributor.author | Manchester, R. N. | en_US |
dc.contributor.author | Torne, P. | en_US |
dc.contributor.author | Sarkissian, J. | en_US |
dc.contributor.author | Heinke, C. O. | en_US |
dc.contributor.author | D'Amico, N. | en_US |
dc.contributor.author | Camilo, F. | en_US |
dc.contributor.author | Lorimer, D. R. | en_US |
dc.contributor.author | Lyne, A. G. | en_US |
dc.date.accessioned | 2021-04-23T13:04:53Z | - |
dc.date.available | 2021-04-23T13:04:53Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30880 | - |
dc.description.abstract | This paper is the second in a series where we report the results of the long-term timing of the millisecond pulsars (MSPs) in 47 Tucanae with the Parkes 64-m radio telescope. We obtain improved timing parameters that provide additional information for studies of the cluster dynamics: (a) the pulsar proper motions yield an estimate of the proper motion of the cluster as a whole (μ<SUB>α</SUB> = 5.00 ± 0.14 mas yr<SUP> - 1</SUP>, μ<SUB>δ</SUB> = - 2.84 ± 0.12 mas yr<SUP> - 1</SUP>) and the motion of the pulsars relative to each other. (b) We measure the second spin-period derivatives caused by the change of the pulsar line-of-sight accelerations; 47 Tuc H, U and possibly J are being affected by nearby objects. (c) For 10 binary systems, we now measure changes in the orbital period caused by their acceleration in the gravitational field of the cluster. From all these measurements, we derive a cluster distance no smaller than ∼4.69 kpc and show that the characteristics of these MSPs are very similar to their counterparts in the Galactic disc. We find no evidence in favour of an intermediate mass black hole at the centre of the cluster. Finally, we describe the orbital behaviour of four 'black widow' systems. Two of them, 47 Tuc J and O, exhibit orbital variability similar to that observed in other such systems, while for 47 Tuc I and R the orbits seem to be remarkably stable. It appears therefore that not all 'black widows' have unpredictable orbital behaviour. | en_US |
dc.language.iso | eng | en_US |
dc.title | Long-term observations of the pulsars in 47 Tucanae - II. Proper motions, accelerations and jerks | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stx1533 | en_US |
dc.identifier.scopus | 2-s2.0-85039415224 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/471/1/857/3869631 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 471 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 857 | 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 | 2017MNRAS.471..857F | 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_11 Relativistic astrophysics | 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.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0001-6762-2638 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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2017_Freire_Ridolfi_etal.pdf | Pdf editoriale | 1.16 MB | Adobe PDF | View/Open |
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Items in DSpace are published in Open Access, unless otherwise indicated.