Search for TeV emission from 4U 0115 + 63

Details Search for TeV emission from 4U 0115 + 63 Search for TeV emission from 4U 0115 + 63

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...376..738m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 376, Aug. 1, 1991, p. 738-745. Research supported by DOE, Irish Scientific

Computer Science

6

Gamma Ray Bursts, Pulsars, X Ray Binaries, Gamma Ray Telescopes, Neutron Stars

Scientific paper

While previous studies of the X-ray binary 4U 0115+63 suggest it to be a steady, TeV gamma-ray emitter, with pulses at the 3.6-sec neutron-star period, the present analysis of data obtained on 60 nights over a 4-yr period with an imaging gamma-ray telescope has uncovered no indication of TeV signals. The derived upper limit of 1 x 10 to the -11th/sq-cm sec, for gamma-rays of energy above 0.7 TeV, is noted to be significantly below the previously reported fluxes.

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