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Volumn 353, Issue 4, 2004, Pages 1286-1292

Three new X-ray pulsars detected in the Small Magellanic Cloud and the positions of two other known pulsars determined

Author keywords

Magellanic Clouds; Stars: emission line, Be; X rays: binaries

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; GALAXIES;

EID: 5644221637     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08150.x     Document Type: Article
Times cited : (31)

References (23)
  • 2
    • 0001517955 scopus 로고    scopus 로고
    • Smith M. A., Henrichs H. F., Fabregat J., eds, The Be Phenomenon in Early-Type Stars. Astron. Soc. Pac., San Francisco
    • Coe M. J., 2000, in Smith M. A., Henrichs H. F., Fabregat J., eds, ASP Conf. Ser. Vol. 214, The Be Phenomenon in Early-Type Stars. Astron. Soc. Pac., San Francisco, p. 656
    • (2000) ASP Conf. Ser. , vol.214 , pp. 656
    • Coe, M.J.1
  • 15
    • 3142554342 scopus 로고    scopus 로고
    • Negueruela I., 1998, A&A, 338, 505
    • (1998) A&A , vol.338 , pp. 505
    • Negueruela, I.1
  • 23
    • 5644294918 scopus 로고    scopus 로고
    • Zezas A., McDowell J. C., Hadzidimitriou D., Kalogera V., Fabbiano G., Taylor P., 2003, preprint (astro-ph/0310562)
    • Zezas A., McDowell J. C., Hadzidimitriou D., Kalogera V., Fabbiano G., Taylor P., 2003, preprint (astro-ph/0310562)


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.