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Volumn 338, Issue 2, 2003, Pages 428-432

Optical counterparts to four X-ray sources in the Small Magellanic Cloud

Author keywords

Magellanic clouds; Stars: General; X rays: Binaries

Indexed keywords

GALAXIES; PHOTOMETRY; SPECTROSCOPIC ANALYSIS; STARS; X RAY APPARATUS;

EID: 0037736356     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06061.x     Document Type: Article
Times cited : (23)

References (24)
  • 1
    • 0001517955 scopus 로고    scopus 로고
    • The Be Phenomenon in Early-Type Stars. Astron. Soc. Pac., San Francisco
    • Coe M.J., 2000, 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
  • 13
    • 3142554342 scopus 로고    scopus 로고
    • Negueruela I., 1998, A&A, 338, 505-510
    • (1998) A&A , vol.338 , pp. 505-510
    • Negueruela, I.1
  • 15


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.