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The same physics underlying SGRs, AXPs and radio pulsars
Gong, Biping
2006
Source PublicationCHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
ISSN1009-9271
Volume6Issue:S2Pages:273-278
Contribution Rank1
Abstract

Unexpected sign, significant magnitude and variable frequency second derivative exists not only in singular radio pulsars but also in Soft Gamma repeaters (SGRs) and Anomalous X-ray pulsars (AXPs). This paper shows that these phenomena are related, and can be interpreted by a simple unified model, long-term orbital effect. Thus many of previous "isolated" pulsars may be binary pulsars, i.e., orbital period P-b approximate to (47, 72)min for AXP 1E 2259+586, and P-b approximate to (20,34)min for PSR J1614-5047, P-b approximate to(3.6,6.4)min for SGR 1900+14, and P-b approximate to (1.5, 5.8)min for SGR 1806-20. In this model, the frequency first derivative of these pulsars is still dominated by magnetic dipole radiation. Therefore, it is not contradictory to the magnetar interpretation of SGRs and AXPs. In other words, the model of this paper provides new interpretation to higher order of derivatives of pulse frequency (second and third...) instead of the first.

KeywordPulsars : Binary Pulsars Timing Noise : Individual (1e 2259+586 Sgr 1806-20 Sgr 1900+14 Psr J1341-6220 Psr J1614-5047)
SubtypeArticle
Subject Area致密天体、高能和基础物理
WOS HeadingsScience & Technology ; Physical Sciences
URL查看原文
Indexed BySCI ; CPCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000245632000054
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Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/196
Collection其它
Corresponding AuthorGong, Biping
AffiliationChinese Acad Sci, Natl Astron Observ, Urumqi Observ, Urumqi 830011, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Corresponding Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Gong, Biping. The same physics underlying SGRs, AXPs and radio pulsars[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2006,6(S2):273-278.
APA Gong, Biping.(2006).The same physics underlying SGRs, AXPs and radio pulsars.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,6(S2),273-278.
MLA Gong, Biping."The same physics underlying SGRs, AXPs and radio pulsars".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 6.S2(2006):273-278.
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