Time Distributions for Underground Muons from the Direction of Cygnus X-3

M. L. Marshak; J. Bartelt; H. Courant; K. Heller; S. Heppelmann; T. Joyce; E. A. Peterson; K. Ruddick; M. Shupe; D. S. Ayres; J. Dawson; T. Fields; E. N. May; L. E. Price; K. Sivaprasad

doi:10.1103/PhysRevLett.55.1965

Time Distributions for Underground Muons from the Direction of Cygnus X-3

M. L. Marshak, J. Bartelt, H. Courant, K. Heller, S. Heppelmann, T. Joyce, E. A. Peterson, K. Ruddick, M. Shupe, D. S. Ayres, J. Dawson, T. Fields, E. N. May, L. E. Price, K. Sivaprasad

Physics and Astronomy (Twin Cities)

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43 Scopus citations

Abstract

Analysis of underground muon events from the direction of Cygnus X-3 shows evidence for large time variability of the flux in addition to the 4.8-h modulation. Our data support earlier suggestions that high fluxes occur with a 34.1-d cycle. Events measured during high-rate periods show increased statistical support for the hypothesis linking underground muons with this x-ray binary.

Original language	English (US)
Pages (from-to)	1965-1968
Number of pages	4
Journal	Physical review letters
Volume	55
Issue number	19
DOIs	https://doi.org/10.1103/PhysRevLett.55.1965
State	Published - 1985

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Marshak, M. L., Bartelt, J., Courant, H., Heller, K., Heppelmann, S., Joyce, T., Peterson, E. A., Ruddick, K., Shupe, M., Ayres, D. S., Dawson, J., Fields, T., May, E. N., Price, L. E., & Sivaprasad, K. (1985). Time Distributions for Underground Muons from the Direction of Cygnus X-3. Physical review letters, 55(19), 1965-1968. https://doi.org/10.1103/PhysRevLett.55.1965

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doi = "10.1103/PhysRevLett.55.1965",

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AU - Marshak, M. L.

AU - Bartelt, J.

AU - Courant, H.

AU - Heller, K.

AU - Heppelmann, S.

AU - Joyce, T.

AU - Peterson, E. A.

AU - Ruddick, K.

AU - Shupe, M.

AU - Ayres, D. S.

AU - Dawson, J.

AU - Fields, T.

AU - May, E. N.

AU - Price, L. E.

AU - Sivaprasad, K.

PY - 1985

Y1 - 1985

N2 - Analysis of underground muon events from the direction of Cygnus X-3 shows evidence for large time variability of the flux in addition to the 4.8-h modulation. Our data support earlier suggestions that high fluxes occur with a 34.1-d cycle. Events measured during high-rate periods show increased statistical support for the hypothesis linking underground muons with this x-ray binary.

AB - Analysis of underground muon events from the direction of Cygnus X-3 shows evidence for large time variability of the flux in addition to the 4.8-h modulation. Our data support earlier suggestions that high fluxes occur with a 34.1-d cycle. Events measured during high-rate periods show increased statistical support for the hypothesis linking underground muons with this x-ray binary.

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DO - 10.1103/PhysRevLett.55.1965

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EP - 1968

JO - Physical review letters

JF - Physical review letters

IS - 19

ER -

Time Distributions for Underground Muons from the Direction of Cygnus X-3

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