A high magnetic field radio pulsar survey with Swift/XRT

Author:

Watanabe Eri1,Shibata Shinpei2,Sakamoto Takanori3,Bamba Aya45

Affiliation:

1. School of Science and Technology, Yamagata University, 1-4-12 Kojirakawa, Yamagata 990-0021, Japan

2. Department of Physics, Yamagata University, 1-4-12 Kojirakawa, Yamagata 990-0021, Japan

3. Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Chuo-ku, Sagamihara, Kanagawa 252-5258, Japan

4. Department of Physics, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

5. Research Center for the Early Universe, School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

Funder

Ministry of Education, Culture, Sports, Science and Technology

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. On the X-ray efficiency of the white dwarf pulsar candidate ZTF J190132.9+145808.7;Publications of the Astronomical Society of Japan;2024-05-23

2. Low X-ray Efficiency of a Young High-B Pulsar PSR J1208−6238 Observed with Chandra;Astrophysics and Space Science;2020-11

3. Is PSR J0726–2612 a dim isolated neutron star progenitor?;Monthly Notices of the Royal Astronomical Society;2020-08-19

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