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    Search for TeV gamma rays from the X-ray pulsar 1E2259+586

    Cawley, Michael F. and Fegan, D.J. and Hillas, A.M. and Kwok, P.W. and Lamb, R.C. and Lang, M.J. and Lewis, D.A. and Macomb, D. and Reynolds, P.T. and Vacanti, G. and Weekes, T.C. (1991) Search for TeV gamma rays from the X-ray pulsar 1E2259+586. Astronomy & Astrophysics, 243 (1). pp. 143-144. ISSN 0004-6361

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    Evidence for TeV gamma-ray emission from 1E2259 + 586 has recently been reported by the Durham Group (Brazier et al., 1990). Evidence suggests that the source is a steady gamma-ray emitter, with a flux an order of magnitude higher than that of the Crab Nebula (Weekes et al., 1989). The Whipple Collaboration observed 1E2259 + 586 for a total of 80 H between November 1985 and November 1988 using the atmospheric Cherenkov imaging technique. These observations, were analysed for evidence of periodic emission at the fundamental and second harmonic of the X-ray period. No evidence for gamma-ray emission from this source is found.

    Item Type: Article
    Keywords: Gamma Ray Spectra; Pulsars; Supernova Remnants; X Ray Sources; Crab Nebula; Gamma Ray Astronomy; Radio Sources (Astronomy); Astrophysics;
    Academic Unit: Faculty of Science and Engineering > Experimental Physics
    Item ID: 12617
    Depositing User: Dr. Michael Cawley
    Date Deposited: 26 Mar 2020 12:26
    Journal or Publication Title: Astronomy & Astrophysics
    Publisher: EDP Sciences
    Refereed: Yes

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