Back to Search Start Over

Discovery and timing of ten new millisecond pulsars in the globular cluster Terzan 5

Authors :
Padmanabh, P. V.
Ransom, S. M.
Freire, P. C. C.
Ridolfi, A.
Taylor, J. D.
Choza, C.
Clark, C. J.
Abbate, F.
Bailes, M.
Barr, E. D.
Buchner, S.
Burgay, M.
DeCesar, M. E.
Chen, W.
Corongiu, A.
Champion, D. J.
Dutta, A.
Geyer, M.
Hessels, J. W. T.
Kramer, M.
Possenti, A.
Stairs, I. H.
Stappers, B. W.
Krishnan, V. Venkatraman
Vleeschower, L.
Zhang, L.
Source :
A&A 686, A166 (2024)
Publication Year :
2024

Abstract

We report the discovery of ten new pulsars in the globular cluster Terzan 5 as part of the Transients and Pulsars with MeerKAT (TRAPUM) Large Survey Project. We observed Terzan 5 at L-band (856--1712 MHz) with the MeerKAT radio telescope for four hours on two epochs, and performed acceleration searches of 45 out of 288 tied-array beams covering the core of the cluster. We obtained phase-connected timing solutions for nine discoveries, covering nearly two decades of archival observations from the Green Bank Telescope for all but one. Highlights include PSR J1748$-$2446ao which is an eccentric ($e = 0.32$) wide-orbit (orbital period $P_{\rm b} = 57.55$ d) system. We were able to measure the rate of advance of periastron ($\dot{\omega}$) for this system allowing us to determine a total mass of $3.17 \pm \, 0.02\, \rm M_{\odot}$. With a minimum companion mass ($M_{\rm c}$) of $\sim 0.8\, \rm M_{\odot}$, PSR J1748$-$2446ao is a candidate double neutron star (DNS) system. If confirmed to be a DNS, it would be the fastest spinning pulsar ($P = 2.27$ ms) and the longest orbital period measured for any known DNS system. PSR J1748$-$2446ap has the second highest eccentricity for any recycled pulsar ($e \sim 0.905$) and for this system we can measure the total mass ($1.997 \pm 0.006\, \rm M_{\odot}$) and also estimate the individual pulsar and companion masses. PSR J1748$-$2446ar is an eclipsing redback (minimum $M_{\rm c} \sim 0.34\, \rm M_{\odot}$) system whose properties confirm it to be the counterpart to a previously published source identified in radio and X-ray imaging. With these discoveries, the total number of confirmed pulsars in Terzan 5 is 49, the highest for any globular cluster so far. These discoveries further enhance the rich set of pulsars known in Terzan 5 and provide scope for a deeper understanding of binary stellar evolution, cluster dynamics and ensemble population studies.<br />Comment: 23 pages, 11 figures, 5 tables, published in A&A

Details

Database :
arXiv
Journal :
A&A 686, A166 (2024)
Publication Type :
Report
Accession number :
edsarx.2403.17799
Document Type :
Working Paper
Full Text :
https://doi.org/10.1051/0004-6361/202449303