4.7 Article

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

期刊

出版社

WILEY-BLACKWELL
DOI: 10.1111/j.1365-2966.2011.19842.x

关键词

pulsars: general; pulsars: individual: PSR J1017-7156; pulsars: individual: PSR J1446-4701; pulsars: individual: PSR J1502-6752

资金

  1. Commonwealth of Australia for operation as a National Facility managed by CSIRO
  2. National Aeronautics and Space Administration
  3. Department of Energy in the United States
  4. Commissariat a l'Energie Atomique
  5. Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France
  6. Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica Nucleare in Italy
  7. Ministry of Education, Culture, Sports, Science and Technology (MEXT)
  8. High Energy Accelerator Research Organization (KEK)
  9. Japan Aerospace Exploration Agency (JAXA) in Japan
  10. K. A. Wallenberg Foundation
  11. Swedish Research Council
  12. Swedish National Space Board in Sweden
  13. Istituto Nazionale di Astrofisica in Italy
  14. Centre National d'Etudes Spatiales in France
  15. Science and Technology Facilities Council [ST/G002487/1, ST/I001131/1, ST/J001562/1, ST/F002874/1] Funding Source: researchfish
  16. STFC [ST/F002874/1, ST/I001131/1, ST/J001562/1, ST/G002487/1] Funding Source: UKRI

向作者/读者索取更多资源

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. PSR J1446-4701 and PSR 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.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.7
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据