Shaifullah, G.G.ShaifullahVerbiest, J. P. W.J. P. W.VerbiestFreire, P. C. C.P. C. C.FreireTauris, T. M.T. M.TaurisWex, N.N.WexOsłowski, S.S.OsłowskiStappers, B. W.B. W.StappersBassa, C. G.C. G.BassaCaballero, R. N.R. N.CaballeroChampion, D. J.D. J.ChampionCognard, I.I.CognardDesvignes, G.G.DesvignesGraikou, E.E.GraikouGuillemot, L.L.GuillemotJanssen, G. H.G. H.JanssenJessner, A.A.JessnerJordan, C.C.JordanKaruppusamy, R.R.KaruppusamyKramer, M.M.KramerLazaridis, K.K.LazaridisLazarus, P.P.LazarusLyne, A. G.A. G.LyneMcKee, J. W.J. W.McKeePERRODIN, DELPHINEDELPHINEPERRODIN0000-0002-1806-2483POSSENTI, ANDREAANDREAPOSSENTI0000-0001-5902-3731Tiburzi, C.C.Tiburzi2020-04-302020-04-3020160035-8711http://hdl.handle.net/20.500.12386/24370Timing results for the black-widow pulsar J2051-0827 are presented, using a 21 year data set from four European Pulsar Timing Array telescopes and the Parkes radio telescope. This data set, which is the longest published to date for a black-widow system, allows for an improved analysis that addresses previously unknown biases. While secular variations, as identified in previous analyses, are recovered, short-term variations are detected for the first time. Concurrently, a significant decrease of ∼ 2.5 × 10<SUP>- 3</SUP> cm<SUP>- 3</SUP> pc in the dispersion measure associated with PSR J2051-0827 is measured for the first time and improvements are also made to estimates of the proper motion. Finally, PSR J2051-0827 is shown to have entered a relatively stable state suggesting the possibility of its eventual inclusion in pulsar timing arrays.STAMPAen21 year timing of the black-widow pulsar J2051-0827Article10.1093/mnras/stw17372-s2.0-84988719640000383516700105https://academic.oup.com/mnras/article/462/1/1029/2589997https://arxiv.org/pdf/1607.04167.pdf2016MNRAS.462.1029SFIS/05 - ASTRONOMIA E ASTROFISICAScienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_6 Stars and stellar systems