A search for TeV emission from cygnus X-3

K. S. O'Flaherty; M. F. Cawley; D. J. Fegan; R. C. Lamb; M. J. Lang; D. A. Lewis; M. Punch; P. T. Reynolds; G. Vacanti; T. C. Weekes

doi:10.1086/171748

A search for TeV emission from cygnus X-3

K. S. O'Flaherty, M. F. Cawley, D. J. Fegan, R. C. Lamb, M. J. Lang, D. A. Lewis, M. Punch, P. T. Reynolds, G. Vacanti, T. C. Weekes

Physics

Research output: Contribution to a Journal (Peer & Non Peer) › Article › peer-review

23 Citations (Scopus)

Abstract

Cygnus X-3 has been observed during 1988-1990 by the Whipple Observatory collaboration using the 109 pixel high-resolution γ-ray imaging telescope. The data recorded has been analyzed to search for (a) steady emission of TeV γ-rays, (b) 4.8 hr modulation of the γ-ray light curve, and (c) periodic emission at 12.59 ms. No evidence is found for emission based on these searches. The upper limit (3 a) for long-term steady emission is 3.5 × 10^-12 photons cm^-2 s^-1, a factor of 10 below fluxes reported a decade ago for this energy.

Original language	English
Pages (from-to)	674-678
Number of pages	5
Journal	Astrophysical Journal
Volume	396
Issue number	2
DOIs	https://doi.org/10.1086/171748
Publication status	Published - 1992

Keywords

Gamma rays: observations
Stars: individual (Cyg X-3)

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10.1086/171748

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@article{02290674c7ae4a6ea5113354ce183b54,

title = "A search for TeV emission from cygnus X-3",

abstract = "Cygnus X-3 has been observed during 1988-1990 by the Whipple Observatory collaboration using the 109 pixel high-resolution γ-ray imaging telescope. The data recorded has been analyzed to search for (a) steady emission of TeV γ-rays, (b) 4.8 hr modulation of the γ-ray light curve, and (c) periodic emission at 12.59 ms. No evidence is found for emission based on these searches. The upper limit (3 a) for long-term steady emission is 3.5 × 10-12 photons cm-2 s-1, a factor of 10 below fluxes reported a decade ago for this energy.",

keywords = "Gamma rays: observations, Stars: individual (Cyg X-3)",

author = "O'Flaherty, \{K. S.\} and Cawley, \{M. F.\} and Fegan, \{D. J.\} and Lamb, \{R. C.\} and Lang, \{M. J.\} and Lewis, \{D. A.\} and M. Punch and Reynolds, \{P. T.\} and G. Vacanti and Weekes, \{T. C.\}",

year = "1992",

doi = "10.1086/171748",

language = "English",

volume = "396",

pages = "674--678",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

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TY - JOUR

T1 - A search for TeV emission from cygnus X-3

AU - O'Flaherty, K. S.

AU - Cawley, M. F.

AU - Fegan, D. J.

AU - Lamb, R. C.

AU - Lang, M. J.

AU - Lewis, D. A.

AU - Punch, M.

AU - Reynolds, P. T.

AU - Vacanti, G.

AU - Weekes, T. C.

PY - 1992

Y1 - 1992

N2 - Cygnus X-3 has been observed during 1988-1990 by the Whipple Observatory collaboration using the 109 pixel high-resolution γ-ray imaging telescope. The data recorded has been analyzed to search for (a) steady emission of TeV γ-rays, (b) 4.8 hr modulation of the γ-ray light curve, and (c) periodic emission at 12.59 ms. No evidence is found for emission based on these searches. The upper limit (3 a) for long-term steady emission is 3.5 × 10-12 photons cm-2 s-1, a factor of 10 below fluxes reported a decade ago for this energy.

AB - Cygnus X-3 has been observed during 1988-1990 by the Whipple Observatory collaboration using the 109 pixel high-resolution γ-ray imaging telescope. The data recorded has been analyzed to search for (a) steady emission of TeV γ-rays, (b) 4.8 hr modulation of the γ-ray light curve, and (c) periodic emission at 12.59 ms. No evidence is found for emission based on these searches. The upper limit (3 a) for long-term steady emission is 3.5 × 10-12 photons cm-2 s-1, a factor of 10 below fluxes reported a decade ago for this energy.

KW - Gamma rays: observations

KW - Stars: individual (Cyg X-3)

UR - https://www.scopus.com/pages/publications/0037776435

U2 - 10.1086/171748

DO - 10.1086/171748

M3 - Article

SN - 0004-637X

VL - 396

SP - 674

EP - 678

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

ER -

A search for TeV emission from cygnus X-3

Abstract

Keywords

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