The High Time Resolution Universe Pulsar Survey IV: Discovery and polarimetry of millisecond pulsars

TL;DR

This paper reports the discovery of six millisecond pulsars in the HTRU survey, analyzes their properties including polarisation, and discusses their potential for precision timing and gamma-ray emission studies.

Contribution

It presents six newly discovered MSPs with detailed polarisation profiles and gamma-ray associations, expanding understanding of MSP emission characteristics and binary properties.

Findings

Six new MSPs discovered in the HTRU survey.

Several MSPs show evidence of pulsed gamma-ray emission.

Many MSPs exhibit complex polarisation profiles with broad emission features.

Abstract

We present the discovery of six millisecond pulsars (MSPs) in the High Time Resolution Universe (HTRU) survey for pulsars and fast transients carried out with the Parkes radio telescope. All six are in binary systems with approximately circular orbits and are likely to have white dwarf companions. PSR J1017-7156 has a high flux density and a narrow pulse width, making it ideal for precision timing experiments. PSRs J1446-4701 and J1125-5825 are coincident with gamma-ray sources, and folding the high-energy photons with the radio timing ephemeris shows evidence of pulsed gamma-ray emission. PSR J1502-6752 has a spin period of 26.7 ms, and its low period derivative implies that it is a recycled pulsar. The orbital parameters indicate it has a very low mass function, and therefore a companion mass much lower than usually expected for such a mildly recycled pulsar. In addition we present polarisation profiles for all 12 MSPs discovered in the HTRU survey to date. Similar to previous observations of MSPs, we find that many have large widths and a wide range of linear and circular polarisation fractions. Their polarisation profiles can be highly complex, and although the observed position angles often do not obey the rotating vector model, we present several examples of those that do. We speculate that the emission heights of MSPs are a substantial fraction of the light cylinder radius in order to explain broad emission profiles, which then naturally leads to a large number of cases where emission from both poles is observed.