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    National Tsing Hua University Institutional Repository > 理學院 > 物理系 > 會議論文  >  ASCA and RXTE upper limits to pulsed emissions from PSR B1951+32


    Please use this identifier to cite or link to this item: http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/56204


    Title: ASCA and RXTE upper limits to pulsed emissions from PSR B1951+32
    Authors: Chang Hsiangkuang;Guo Tzfeng
    教師: 張祥光
    Date: 2000
    Publisher: American Society of Primatologists
    Relation: Astronomical Society of the Pacific Conference Series, European Space Agency, Volume 202, 2000, Pages 327-328
    Keywords: gamma-ray sources
    pulsars
    stellar pulsations
    stellar radiation
    Abstract: We report upper limits to pulsed X-ray emissions from PSR B1951+32 in 0.5-250 keV based on observations of ASCA in 1993 and RXTE in 1996. Together with earlier ROSAT report, these upper limits strongly suggest a thermal pulsed component below about 1 keV. These upper limits also indicate a spectral bending occurring in 100 keV-3 MeV, which favors an outer-magnetosphere origin for gamma-ray emissions from PSR B1951+32
    URI: http://adsabs.harvard.edu/full/2000ASPC..202..327C
    http://www.asp.org/
    http://nthur.lib.nthu.edu.tw/dspace/handle/987654321/56204
    Appears in Collections:[物理系] 會議論文

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