A multiwavelength search for black widow and redback counterparts of candidate γ-ray millisecond pulsars

Author:

Braglia C1,Mignani R P23ORCID,Belfiore A2,Marelli M2,Israel G L4,Novara G25,De Luca A26,Tiengo A256ORCID,Saz Parkinson P M78

Affiliation:

1. Department of Physics ‘A. Pontremoli’, University of Milan, via G. Celoria 16, I-20133 Milan, Italy

2. INAF – Istituto di Astrofisica Spaziale e Fisica Cosmica Milano, via A. Corti 12, I-20133 Milan, Italy

3. Janusz Gil Institute of Astronomy, University of Zielona Góra, ul Szafrana 2, PL-65-265 Zielona Góra, Poland

4. INAF – Osservatorio Astronomico di Roma, via Frascati 33, I-00040 Monteporzio Catone, Italy

5. Scuola Universitaria Superiore IUSS Pavia, Piazza della Vittoria 15, I-27100 Pavia, Italy

6. INFN, Sezione di Pavia, via A. Bassi 6, I-27100 Pavia, Italy

7. Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, CA 95064, USA

8. Department of Physics, Laboratory for Space Research, University of Hong Kong, Pokfulam Road, Hong Kong

Abstract

ABSTRACT The wealth of detections of millisecond pulsars (MSPs) in γ-rays by Fermi has spurred searches for these objects among the several unidentified γ-ray sources. Interesting targets are a sub-class of binary MSPs, dubbed ‘black widows’ (BWs) and ‘redbacks’ (RBs), which are in orbit with low-mass non-degenerate companions fully or partially ablated by irradiation from the MSP wind. These systems can be easily missed in radio pulsar surveys owing to the eclipse of the radio signal by the intra-binary plasma from the ablated companion star photosphere, making them better targets for multiwavelength observations. We used optical and X-ray data from public data bases to carry out a systematic investigation of all the unidentified γ-ray sources from the Fermi Large Area Telescope Third Source Catalog, which have been pre-selected as likely MSP candidates according to a machine-learning technique analysis. We tested our procedure by recovering known binary BW/RB identifications and searched for new ones, finding two possible candidates. At the same time, we investigated previously proposed BW/RB identifications and we ruled out one of them based upon the updated γ-ray source coordinates.

Funder

National Aeronautics and Space Administration

National Science Foundation

Seventh Framework Programme

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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