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Volumn 529, Issue , 2011, Pages

The Swift-BAT survey reveals the orbital period of three high-mass X-ray binaries

Author keywords

X rays: binaries; X rays: individuals: IGRJ05007 7047; X rays: individuals: IGRJ13186 6257; X rays: individuals: IGRJ17354 3255

Indexed keywords

ENERGY BAND; ENERGY SPECTRA; FOLDING TECHNIQUE; INTEGRAL SOURCES; LARGE MAGELLANIC CLOUDS; LIGHT CURVES; NEW SOURCES; ORBITAL PERIODS; PERIOD SEARCH; PERIODOGRAMS; SOFT X-RAY; SWIFT SATELLITES; X RAY BINARIES; X-RAY EMISSION; X-RAY SOURCES; X-RAY SPECTRAL EMISSIONS; X-RAYS: BINARIES; X-RAYS: INDIVIDUAL; X-RAYS: INDIVIDUALS: IGRJ17354-3255;

EID: 79953136082     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016401     Document Type: Article
Times cited : (35)

References (30)
  • 3
    • 79952462607 scopus 로고
    • ed. V. di Gesu L. Scarsi, P. Crane, J. H. Friedman, & S. Levialdi
    • Buccheri, R., & Sacco, B. 1985, in Data Analysis in Astronomy, ed. V. di Gesu, L. Scarsi, P. Crane, J. H. Friedman, & S. Levialdi, 15
    • (1985) Data Analysis in Astronomy , pp. 15
    • Buccheri, R.1    Sacco, B.2
  • 5
    • 79953145354 scopus 로고    scopus 로고
    • Chaty, S., Zurita Heras, J. A., & Bodaghee, A. 2010 [arXiv:1012.2318]
    • Chaty, S., Zurita Heras, J. A., & Bodaghee, A. 2010 [arXiv:1012.2318]


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.