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TeV gamma-ray emission from binaries: 2129+47XR and Cygnus X-3

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Title: TeV gamma-ray emission from binaries: 2129+47XR and Cygnus X-3
Authors: Sinitsyna, V.G.1, Arsov, T.P.1, Alaverdian, A.Y.1, Borisov, S.S.1, Mirzafatikhov, R.M.1, Musin, F.I.1, Nikolsky, S.I.1, Sinitsyna, V.Y.1, Platonov, G.F.1, Capdevielle, J.-N.2
Source: Nuclear Physics B Proceedings Supplement. Jan2008, Vol. 175-176 Issue 1, p544-547. 4p.
Subjects: Spectrum analysis, Particles (Nuclear physics), Nuclear physics, Physics
Abstract: The new galactic gamma-source (neutron star) 2129+47XR is detected at energy with flux and indices of the integral spectra are , and . The results of ten-year observation of galactic source Cygnus X-3 by SHALON mirror Cherenkov telescope are discussed. The gamma -quantum spectra and images of the sources are presented. The Cygnus X-3 binary, known for more than 20 years as a source with variable intensity have been regularly observed since a 1995. The the increase of gamma-quantum flux was observed in 1997 and 2003 years. [Copyright &y& Elsevier]
Copyright of Nuclear Physics B Proceedings Supplement is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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DbLabel: Engineering Source
An: 28154379
AccessLevel: 6
PubType: Periodical
PubTypeId: serialPeriodical
PreciseRelevancyScore: 0
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  Data: TeV gamma-ray emission from binaries: 2129+47XR and Cygnus X-3
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  Data: <searchLink fieldCode="AR" term="%22Sinitsyna%2C+V%2EG%2E%22">Sinitsyna, V.G.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Arsov%2C+T%2EP%2E%22">Arsov, T.P.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Alaverdian%2C+A%2EY%2E%22">Alaverdian, A.Y.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Borisov%2C+S%2ES%2E%22">Borisov, S.S.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Mirzafatikhov%2C+R%2EM%2E%22">Mirzafatikhov, R.M.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Musin%2C+F%2EI%2E%22">Musin, F.I.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Nikolsky%2C+S%2EI%2E%22">Nikolsky, S.I.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Sinitsyna%2C+V%2EY%2E%22">Sinitsyna, V.Y.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Platonov%2C+G%2EF%2E%22">Platonov, G.F.</searchLink><relatesTo>1</relatesTo><br /><searchLink fieldCode="AR" term="%22Capdevielle%2C+J%2E-N%2E%22">Capdevielle, J.-N.</searchLink><relatesTo>2</relatesTo>
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  Data: <searchLink fieldCode="JN" term="%22Nuclear+Physics+B++Proceedings+Supplement%22">Nuclear Physics B Proceedings Supplement</searchLink>. Jan2008, Vol. 175-176 Issue 1, p544-547. 4p.
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  Data: <searchLink fieldCode="DE" term="%22Spectrum+analysis%22">Spectrum analysis</searchLink><br /><searchLink fieldCode="DE" term="%22Particles+%28Nuclear+physics%29%22">Particles (Nuclear physics)</searchLink><br /><searchLink fieldCode="DE" term="%22Nuclear+physics%22">Nuclear physics</searchLink><br /><searchLink fieldCode="DE" term="%22Physics%22">Physics</searchLink>
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  Label: Abstract
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  Data: The new galactic gamma-source (neutron star) 2129+47XR is detected at energy with flux and indices of the integral spectra are , and . The results of ten-year observation of galactic source Cygnus X-3 by SHALON mirror Cherenkov telescope are discussed. The gamma -quantum spectra and images of the sources are presented. The Cygnus X-3 binary, known for more than 20 years as a source with variable intensity have been regularly observed since a 1995. The the increase of gamma-quantum flux was observed in 1997 and 2003 years. [Copyright &y& Elsevier]
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  Data: <i>Copyright of Nuclear Physics B Proceedings Supplement is the property of Elsevier B.V. and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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      – TitleFull: TeV gamma-ray emission from binaries: 2129+47XR and Cygnus X-3
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              Text: Jan2008
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