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Volumn 442, Issue 3, 2005, Pages 1135-1138

High-mass X-ray binaries in the Magellanic Clouds

Author keywords

Catalogs; Magellanic Clouds; Stars: early type; X rays: binaries

Indexed keywords

INFRARED RADIATION; PARAMETER ESTIMATION; SPECTRUM ANALYSIS; ULTRAVIOLET RADIATION;

EID: 27344437210     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20053718     Document Type: Article
Times cited : (103)

References (34)
  • 2
    • 0001517955 scopus 로고    scopus 로고
    • The Be Phenomenon in Early-Type Stars, ed. M. A. Smith, & H. F. Henrichs (San Francisco: ASP)
    • Coe, M. J. 2000, in The Be Phenomenon in Early-Type Stars, ed. M. A. Smith, & H. F. Henrichs (San Francisco: ASP), IAU Colloq., 175, 656
    • (2000) IAU Colloq. , vol.175 , pp. 656
    • Coe, M.J.1
  • 11
    • 0036606992 scopus 로고    scopus 로고
    • Kahabka, P. 2002, A&A, 388, 100
    • (2002) A&A , vol.388 , pp. 100
    • Kahabka, P.1
  • 22
  • 30
    • 0001803945 scopus 로고
    • ed. W. H. G. Lewin, J. Van Paradijs, & E. P. J. van den Heuvel, Cambridge
    • Van Paradijs, J. 1995, in X-ray Binaries, ed. W. H. G. Lewin, J. Van Paradijs, & E. P. J. van den Heuvel, Cambridge, 536
    • (1995) X-ray Binaries , pp. 536
    • Van Paradijs, J.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.