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Volumn 330, Issue 6006, 2010, Pages 944-946

A low-magnetic-field soft gamma repeater

Author keywords

[No Author keywords available]

Indexed keywords

EXPERIMENTAL STUDY; GAMMA RAY RADIATION; MAGNETIC FIELD; NEUTRON ACTIVATION ANALYSIS;

EID: 78149415743     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1196088     Document Type: Article
Times cited : (337)

References (31)
  • 1
    • 78149411956 scopus 로고    scopus 로고
    • We note that the surface dipolar magnetic field of magnetars has been estimated also with several other methods (6, 22, 28); these give values consistent with those derived from the formula in Eq. 1
    • We note that the surface dipolar magnetic field of magnetars has been estimated also with several other methods (6, 22, 28); these give values consistent with those derived from the formula in Eq. 1.
  • 3
    • 78149415169 scopus 로고    scopus 로고
    • See for an updated catalog of SGRs and AXPs
    • See www.physics.mcgill.ca/~pulsar/magnetar/main.html for an updated catalog of SGRs and AXPs.
  • 8
    • 41349095225 scopus 로고    scopus 로고
    • F. P. Gavriil et al., Science 319, 1802 (2008).
    • (2008) Science , vol.319 , pp. 1802
    • Gavriil, F.P.1
  • 11
    • 33747845862 scopus 로고    scopus 로고
    • F. Camilo et al., Nature 442, 892 (2006).
    • (2006) Nature , vol.442 , pp. 892
    • Camilo, F.1
  • 18
    • 77956082442 scopus 로고    scopus 로고
    • W. Becker, Ed. Springer, Berlin
    • R. Turolla, in Neutron Stars and Pulsars, W. Becker, Ed. (Springer, Berlin, 2009), pp. 141-164.
    • (2009) Neutron Stars and Pulsars , pp. 141-164
    • Turolla, R.1
  • 26
    • 78149415628 scopus 로고    scopus 로고
    • 14 G (6)
    • 14 G (6).
  • 27
    • 78149415562 scopus 로고    scopus 로고
    • If fast-spinning young pulsars were among these, the resulting magnetically induced ellipticity would lead to powerful emission of periodic gravitational waves
    • If fast-spinning young pulsars were among these, the resulting magnetically induced ellipticity would lead to powerful emission of periodic gravitational waves.
  • 31
    • 78149414031 scopus 로고    scopus 로고
    • note
    • N.R. is supported by a Ramón y Cajal fellowship through Consejo Superior de Investigaciones Cientfícas and by grants AYA2009-07391 and SGR2009-811. N.R. thanks D. F. Torres for useful discussions. P.E. acknowledges financial support from the Autonomous Region of Sardinia through a research grant under the program PO Sardegna FSE 2007-2013, L.R. 7/2007 "Promoting scientific research and innovation technology in Sardinia." D.G. acknowledges the Centre National d'Études Spatiales for financial support. The work of R.T., G.L.I., L.S., S.M., and A.T. is partially supported by INAF Agenzia Spaziale Italiana through grant AAE I/088/06/0. We are grateful to H. Tananbaum, N. Gehrels, and N. Schartel for granting us Chandra, Swift, and XMM-Newton time, respectively, for this research.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.