XAO OpenIR  > 射电天文研究室  > 脉冲星研究团组
Mutual Influence of Magnetic Field Decay and Thermal Evolution of Rotational Neutron Stars
Zhou, Xia1; Kang, Miao2; Wang, Na1
2012
Conference NameInternational Conference on Electromagnetic Radiation from Pulsars and Magnetars (ERPM)
Source PublicationProceeding of Electromagnetic Radiation from Pulsars and Magnetars, ASP Conference Series,466,233-234
Pages233-234
Conference DateAPR 24-27, 2012
Conference PlaceUniv Zielona Gora, Zielona Gora, POLAND
Publication PlaceSAN FRANCISCO, CA 94112 USA
PublisherASTRONOMICAL SOC PACIFIC, 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA
Contribution Rank1
Abstract

Magnetic field decay, rotation and thermal evolution of neutron stars are. interdependent and should be considered together. The results show that magnetic field decay is delayed significantly relative to stars cooling without heating; compared to typical chemical heating, the decay of the magnetic field can even cause the temperature turns down at later stage; and the spin down is also turned slow at photon cooling era.

Funding OrganizationKepler Inst Astron ; City Off Zielona Gora ; Kepler Inst Astron ; City Off Zielona Gora
Subject Area致密天体、高能和基础物理
URL查看原文
Indexed ByCPCI
Funding Project脉冲星研究团组
Language英语
ISBN978-1-58381-814-5
Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/399
Collection射电天文研究室_脉冲星研究团组
射电天文研究室
其它
Corresponding AuthorZhou, Xia
Affiliation1.Xinjiang Astronomical Observatory, CAS, 150, Science 1-Street, Urumqi, 830011, China
2.College of Physics and Electronics, Henan University, Kaifeng, 475004, China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhou, Xia,Kang, Miao,Wang, Na. Mutual Influence of Magnetic Field Decay and Thermal Evolution of Rotational Neutron Stars[C]. SAN FRANCISCO, CA 94112 USA:ASTRONOMICAL SOC PACIFIC, 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA,2012:233-234.
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