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Volumn 387, Issue 2, 2008, Pages 724-728

An optical and X-ray study of the counterpart to the Small Magellanic Cloud X-ray binary pulsar system SXP327

Author keywords

Stars: neutron; X rays: binaries

Indexed keywords

PULSARS;

EID: 45149114280     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13257.x     Document Type: Article
Times cited : (13)

References (17)
  • 1
    • 0001517955 scopus 로고    scopus 로고
    • in. Smith, M. A., Henrichs, H. F., eds, Proc. IAU Colloq. 175, ASP Conf. Ser. Vol. 214, Astron. Soc. Pac., San Francisco, p.
    • Coe M. J., 2000, in Smith M. A., Henrichs H. F., eds, Proc. IAU Colloq. 175, ASP Conf. Ser. Vol. 214, The Be Phenomenon in Early-Type Stars. Astron. Soc. Pac., San Francisco, p. 656
    • (2000) The Be Phenomenon in Early-Type Stars. , pp. 656
    • Coe, M.J.1
  • 7
    • 34547167050 scopus 로고    scopus 로고
    • Kato D. et al., 2007, PASJ, 59, 615
    • (2007) PASJ , vol.59 , pp. 615
    • Kato, D.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.