Serendipitous Discovery of a 431 ms Pulsar in the Background of Westerlund 1

Author:

Piga Viviana12,Burgay Marta1ORCID,Possenti Andrea1,Ridolfi Alessandro1,Pilia Maura1ORCID,Rea Nanda34,Perna Rosalba56ORCID,Colpi Monica78,Israel Gianluca9ORCID

Affiliation:

1. INAF—Osservatorio Astronomico di Cagliari, Via della Scienza 5, I-09047 Selargius, Italy

2. Dipartimento di Matematica e Informatica, Università di Cagliari, Via Ospedale 72, 09124 Cagliari, Italy

3. Institute of Space Sciences (ICE, CSIC), Carrer de Can Magrans, Cerdanyola del Vallès, 08193 Barcelona, Spain

4. Institut d’Estudis Espacials de Catalunya (IEEC), Carrer Gran Capita 2–4, 08034 Barcelona, Spain

5. Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794, USA

6. Center for Computational Astrophysics, Flatiron Institute, New York, NY 10010, USA

7. Dipartimento di Fisica, Università di Milano—Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy

8. Instituto Nazionale di Fisica Nucleare (INFN), Sezione di Milano Bicocca, Milano—Bicocca, Piazza della Scienza 3, I-20126 Milano, Italy

9. INAF—Osservatorio Astronomico di Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy

Abstract

We report the discovery of PSR J1646−4545, a 431 ms isolated pulsar, in the direction of the young massive cluster Westerlund 1. The pulsar was found in data taken between the years 2005 and 2010 with the “Murriyang” Parkes radio telescope in Australia. Thanks to the numerous detections of the pulsar, we were able to derive a phase-connected timing solution spanning the whole data set. This allowed us to precisely locate the pulsar at the border of the cluster and to measure its spin-down rate. The latter implies a characteristic age of ∼25 Myr, about twice as large as the estimated age of Westerlund 1. The age of PSR J1646−4545, together with its dispersion measure of ∼1029 pc cm−3, more than twice the value predicted by the two main galactic electron density models for Westerlund 1, makes the association of the pulsar with the cluster highly unlikely. We also report on ramifications from the presence of a magnetar in Westerlund 1 and the apparent lack of ordinary radio pulsars.

Publisher

MDPI AG

Reference45 articles.

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