Search for γ rays above 1014 eV from Cygnus X-3 during the June and July 1989 radio outbursts
We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as...
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E-Artikel |
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1989 |
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Online-Ressource 4 |
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| Reproduktion: |
APS Digital Backfile Archive 1893-2003 |
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| Übergeordnetes Werk: |
Enthalten in: Physical review letters - College Park, Md. : APS, 1958, 63(1989), 21, Seite 2329-2332 |
| Übergeordnetes Werk: |
volume:63 ; year:1989 ; number:21 ; pages:2329-2332 ; extent:4 |
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| 520 | |a We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1×1014 eV is <5.5×10-13 cm-1 sec-1 (90% C.L.). | ||
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| 700 | 1 | |a Cooper, R. |4 oth | |
| 700 | 1 | |a Corbato, S. C. |4 oth | |
| 700 | 1 | |a Dawson, B. R. |4 oth | |
| 700 | 1 | |a Elbert, J. W. |4 oth | |
| 700 | 1 | |a Fick, B. E. |4 oth | |
| 700 | 1 | |a Green, K. D. |4 oth | |
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| 700 | 1 | |a Liebing, D. F. |4 oth | |
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(DE-627)NLEJ250937638 (DE-601)aps:c4ff2b0733f48bfdb65eb323327b4127e3cb3665 DE-627 ger DE-627 rakwb Search for γ rays above 1014 eV from Cygnus X-3 during the June and July 1989 radio outbursts 1989 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1×1014 eV is <5.5×10-13 cm-1 sec-1 (90% C.L.). APS Digital Backfile Archive 1893-2003 Cassiday, G. L. oth Ciampa, D. oth Cooper, R. oth Corbato, S. C. oth Dawson, B. R. oth Elbert, J. W. oth Fick, B. E. oth Green, K. D. oth Kieda, D. B. oth Ko, S. oth Kolodziejczak, J. oth Liebing, D. F. oth Loh, E. C. oth Matthews, J. oth Nitz, D. oth Salamon, M. H. oth Sinclair, D. oth Smith, J. D. oth Sokolsky, P. oth Thomas, S. B. oth Thornton, G. oth Wheeler, B. oth van der Velde, J. C. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 63(1989), 21, Seite 2329-2332 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:63 year:1989 number:21 pages:2329-2332 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ac4ff2b0733f48bfdb65eb323327b4127e3cb3665 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 1989 21 2329-2332 4 |
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(DE-627)NLEJ250937638 (DE-601)aps:c4ff2b0733f48bfdb65eb323327b4127e3cb3665 DE-627 ger DE-627 rakwb Search for γ rays above 1014 eV from Cygnus X-3 during the June and July 1989 radio outbursts 1989 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1×1014 eV is <5.5×10-13 cm-1 sec-1 (90% C.L.). APS Digital Backfile Archive 1893-2003 Cassiday, G. L. oth Ciampa, D. oth Cooper, R. oth Corbato, S. C. oth Dawson, B. R. oth Elbert, J. W. oth Fick, B. E. oth Green, K. D. oth Kieda, D. B. oth Ko, S. oth Kolodziejczak, J. oth Liebing, D. F. oth Loh, E. C. oth Matthews, J. oth Nitz, D. oth Salamon, M. H. oth Sinclair, D. oth Smith, J. D. oth Sokolsky, P. oth Thomas, S. B. oth Thornton, G. oth Wheeler, B. oth van der Velde, J. C. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 63(1989), 21, Seite 2329-2332 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:63 year:1989 number:21 pages:2329-2332 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ac4ff2b0733f48bfdb65eb323327b4127e3cb3665 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 1989 21 2329-2332 4 |
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(DE-627)NLEJ250937638 (DE-601)aps:c4ff2b0733f48bfdb65eb323327b4127e3cb3665 DE-627 ger DE-627 rakwb Search for γ rays above 1014 eV from Cygnus X-3 during the June and July 1989 radio outbursts 1989 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1×1014 eV is <5.5×10-13 cm-1 sec-1 (90% C.L.). APS Digital Backfile Archive 1893-2003 Cassiday, G. L. oth Ciampa, D. oth Cooper, R. oth Corbato, S. C. oth Dawson, B. R. oth Elbert, J. W. oth Fick, B. E. oth Green, K. D. oth Kieda, D. B. oth Ko, S. oth Kolodziejczak, J. oth Liebing, D. F. oth Loh, E. C. oth Matthews, J. oth Nitz, D. oth Salamon, M. H. oth Sinclair, D. oth Smith, J. D. oth Sokolsky, P. oth Thomas, S. B. oth Thornton, G. oth Wheeler, B. oth van der Velde, J. C. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 63(1989), 21, Seite 2329-2332 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:63 year:1989 number:21 pages:2329-2332 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ac4ff2b0733f48bfdb65eb323327b4127e3cb3665 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 1989 21 2329-2332 4 |
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(DE-627)NLEJ250937638 (DE-601)aps:c4ff2b0733f48bfdb65eb323327b4127e3cb3665 DE-627 ger DE-627 rakwb Search for γ rays above 1014 eV from Cygnus X-3 during the June and July 1989 radio outbursts 1989 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1×1014 eV is <5.5×10-13 cm-1 sec-1 (90% C.L.). APS Digital Backfile Archive 1893-2003 Cassiday, G. L. oth Ciampa, D. oth Cooper, R. oth Corbato, S. C. oth Dawson, B. R. oth Elbert, J. W. oth Fick, B. E. oth Green, K. D. oth Kieda, D. B. oth Ko, S. oth Kolodziejczak, J. oth Liebing, D. F. oth Loh, E. C. oth Matthews, J. oth Nitz, D. oth Salamon, M. H. oth Sinclair, D. oth Smith, J. D. oth Sokolsky, P. oth Thomas, S. B. oth Thornton, G. oth Wheeler, B. oth van der Velde, J. C. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 63(1989), 21, Seite 2329-2332 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:63 year:1989 number:21 pages:2329-2332 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ac4ff2b0733f48bfdb65eb323327b4127e3cb3665 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 1989 21 2329-2332 4 |
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(DE-627)NLEJ250937638 (DE-601)aps:c4ff2b0733f48bfdb65eb323327b4127e3cb3665 DE-627 ger DE-627 rakwb Search for γ rays above 1014 eV from Cygnus X-3 during the June and July 1989 radio outbursts 1989 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1×1014 eV is <5.5×10-13 cm-1 sec-1 (90% C.L.). APS Digital Backfile Archive 1893-2003 Cassiday, G. L. oth Ciampa, D. oth Cooper, R. oth Corbato, S. C. oth Dawson, B. R. oth Elbert, J. W. oth Fick, B. E. oth Green, K. D. oth Kieda, D. B. oth Ko, S. oth Kolodziejczak, J. oth Liebing, D. F. oth Loh, E. C. oth Matthews, J. oth Nitz, D. oth Salamon, M. H. oth Sinclair, D. oth Smith, J. D. oth Sokolsky, P. oth Thomas, S. B. oth Thornton, G. oth Wheeler, B. oth van der Velde, J. C. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 63(1989), 21, Seite 2329-2332 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:63 year:1989 number:21 pages:2329-2332 extent:4 https://www.tib.eu/de/suchen/id/aps%3Ac4ff2b0733f48bfdb65eb323327b4127e3cb3665 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 63 1989 21 2329-2332 4 |
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Cassiday, G. L. @@oth@@ Ciampa, D. @@oth@@ Cooper, R. @@oth@@ Corbato, S. C. @@oth@@ Dawson, B. R. @@oth@@ Elbert, J. W. @@oth@@ Fick, B. E. @@oth@@ Green, K. D. @@oth@@ Kieda, D. B. @@oth@@ Ko, S. @@oth@@ Kolodziejczak, J. @@oth@@ Liebing, D. F. @@oth@@ Loh, E. C. @@oth@@ Matthews, J. @@oth@@ Nitz, D. @@oth@@ Salamon, M. H. @@oth@@ Sinclair, D. @@oth@@ Smith, J. D. @@oth@@ Sokolsky, P. @@oth@@ Thomas, S. B. @@oth@@ Thornton, G. @@oth@@ Wheeler, B. @@oth@@ van der Velde, J. C. @@oth@@ |
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Online-Ressource 4 |
| format_se |
Elektronische Aufsätze |
| title_sort |
search for γ rays above 1014 ev from cygnus x-3 during the june and july 1989 radio outbursts |
| title_auth |
Search for γ rays above 1014 eV from Cygnus X-3 during the June and July 1989 radio outbursts |
| abstract |
We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1×1014 eV is <5.5×10-13 cm-1 sec-1 (90% C.L.). |
| abstractGer |
We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1×1014 eV is <5.5×10-13 cm-1 sec-1 (90% C.L.). |
| abstract_unstemmed |
We have looked for γ-ray emission above 100 TeV from the binary x-ray source Cygnus X-3 during a period of intense radio emission in the summer of 1989. We find no evidence for excess air showers from the direction of the source and the muon content of air showers from this direction is the same as that of ordinary cosmic rays. The flux of γ rays from Cygnus X-3 with energies exceeding 2.1×1014 eV is <5.5×10-13 cm-1 sec-1 (90% C.L.). |
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21 |
| title_short |
Search for γ rays above 1014 eV from Cygnus X-3 during the June and July 1989 radio outbursts |
| url |
https://www.tib.eu/de/suchen/id/aps%3Ac4ff2b0733f48bfdb65eb323327b4127e3cb3665 |
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Cassiday, G. L. Ciampa, D. Cooper, R. Corbato, S. C. Dawson, B. R. Elbert, J. W. Fick, B. E. Green, K. D. Kieda, D. B. Ko, S. Kolodziejczak, J. Liebing, D. F. Loh, E. C. Matthews, J. Nitz, D. Salamon, M. H. Sinclair, D. Smith, J. D. Sokolsky, P. Thomas, S. B. Thornton, G. Wheeler, B. van der Velde, J. C. |
| author2Str |
Cassiday, G. L. Ciampa, D. Cooper, R. Corbato, S. C. Dawson, B. R. Elbert, J. W. Fick, B. E. Green, K. D. Kieda, D. B. Ko, S. Kolodziejczak, J. Liebing, D. F. Loh, E. C. Matthews, J. Nitz, D. Salamon, M. H. Sinclair, D. Smith, J. D. Sokolsky, P. Thomas, S. B. Thornton, G. Wheeler, B. van der Velde, J. C. |
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2024-07-06T09:37:49.622Z |
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