The surface and inner temperatures of magnetars

doi:10.1017/S1743921312024222

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	The surface and inner temperatures of magnetars
	Gao, Z. F.1 ; Wang, N.1 ; Peng, Q. H.2
	2013-02-21
Conference Name	IAU Symposium 291：Neutron Stars and Pulsars: Challenges and Opportunities after 80 years
Source Publication	Neutron Stars and Pulsars: Challenges and Opportunities after 80 years, Proceedings of the International Astronomical Union, IAU Symposium 291
Volume	291
Pages	386-388
Conference Date	20-31 August 2012
Correspondent Email	zhifu_gao@xao.ac.cn ; qhpeng@nju.edu.cn
Conference Place	Beijing, China
Publisher	Cambridge University Press
Project Number	10773005 ; 2012CB821800 ; KJCX2-YW -T09 ; 10173020 ; 10673021 ; 10773005 ; 10778631 ; 10903019
Contribution Rank	1
Abstract	Assuming that the timescale of the magnetic field decay is approximately equal to that of the stellar cooling via neutrino emission, we obtain a one-to-one relationship between the effective surface thermal temperature and the inner temperature. The ratio of the effective neutrino luminosity to the effective X-ray luminosity decreases with decaying magnetic field.
Funding Organization	国家自然科学基金 ; IAU ; 国家自然科学基金 ; IAU ; 973项目 ; 973项目 ; 中国科学院知识创新项目 ; 中国科学院知识创新项目 ; Key Directional Project of CAS ; Key Directional Project of CAS
Keyword	Magnetar Neutrino Luminosity Surface Thermal Temperature Inner Temperature
DOI	10.1017/S1743921312024222
URL	查看原文
Language	英语
ISBN	978-1-107-03380-1
ISSN	2333-9721
Citation statistics
Document Type	会议论文
Identifier	http://ir.xao.ac.cn/handle/45760611-7/979
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 Author	Gao, Z. F.; Peng, Q. H.
Affiliation	1.Xinjiang Astronomical Observatory, CAS, 150, Science 1-Street,Urumqi Xinjiang, 830011, China 2.Shchool of Astronomy and Space Science, Nanjing University,Nanjing Jiangshu, 210093, China
Recommended Citation GB/T 7714	Gao, Z. F.,Wang, N.,Peng, Q. H.. The surface and inner temperatures of magnetars[C]:Cambridge University Press,2013:386-388.

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