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Volumn 356, Issue 3, 2000, Pages 1003-1009

Detection of X-ray pulsations from the Be/X-ray transient A 0535+26 during a disc loss phase of the primary

Author keywords

Stars: binaries: close; Stars: circumstellar matter; Stars: emission line, Be; Stars: individual: A 0535+26; Stars: neutron; X rays: stars

Indexed keywords


EID: 0008575448     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article
Times cited : (54)

References (36)
  • 11
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    • Smith M., Henrichs H.F., Fabregat J. (eds.) The Be Phenomenon in Early-Type Stars. ASP, San Francisco, in press
    • Hanuschik R.W., 2000, In: Smith M., Henrichs H.F., Fabregat J. (eds.) IAU Colloq. 175, The Be Phenomenon in Early-Type Stars. ASP, San Francisco, in press
    • (2000) IAU Colloq. , vol.175
    • Hanuschik, R.W.1
  • 20
  • 23
    • 0000110404 scopus 로고    scopus 로고
    • Okazaki A.T., 1997a, A&A 318, 548
    • (1997) A&A , vol.318 , pp. 548
    • Okazaki, A.T.1
  • 24
    • 3142548548 scopus 로고    scopus 로고
    • Tóth V.L., Kun M., Szabados L. (eds.) Konkoly Observatory, Budapest
    • Okazaki A.T., 1997b, In: Tóth V.L., Kun M., Szabados L. (eds.) The Interaction of Stars with Their Environment. Konkoly Observatory, Budapest, p. 407
    • (1997) The Interaction of Stars with Their Environment , pp. 407
    • Okazaki, A.T.1
  • 25
    • 0000554743 scopus 로고    scopus 로고
    • Porter J.M., 1999, A&A 348, 512
    • (1999) A&A , vol.348 , pp. 512
    • Porter, J.M.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.