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Volumn 326, Issue 5959, 2009, Pages 1512-1516

Modulated high-energy gamma-ray emission from the microquasar Cygnus X-3

(176)  Abdo, A A a,b   Ackermann, M c   Ajello, M c   Axelsson, M d,e   Baldini, L f   Ballet, J g   Barbiellini, G h,i   Bastieri, D j,k   Baughman, B M l   Bechtol, K c   Bellazzini, R f   Berenji, B c   Blandford, R D c   Bloom, E D c   Bonamente, E m,n   Borgland, A W c   Brez, A f   Brigida, M o,p   Bruel, P q   Burnett, T H r   more..


Author keywords

[No Author keywords available]

Indexed keywords

EMISSION; GAMMA RAY RADIATION; JET; PLANETARY ATMOSPHERE;

EID: 72149106222     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1182174     Document Type: Article
Times cited : (286)

References (31)
  • 16
    • 0142132332 scopus 로고    scopus 로고
    • Cambridge Astrophysics Series, no.39, W. H. G. Lewin, M. van der Klis, Eds. Cambridge Univ. Press, Cambridge
    • R. Fender, Compact Stellar X-ray Sources, Cambridge Astrophysics Series, no.39, W. H. G. Lewin, M. van der Klis, Eds. (Cambridge Univ. Press, Cambridge, 2006).
    • (2006) Compact Stellar X-ray Sources
    • Fender, R.1
  • 20
    • 72149089508 scopus 로고    scopus 로고
    • M. Tavani et al., http://lanl.arxiv.org/abs/0910.5344.
    • Tavani, M.1
  • 25
    • 72149085383 scopus 로고    scopus 로고
    • note
    • The orbital modulation on its own does not limit the size of the emitting region to the size of the binary orbit, because the orbital period could be imprinted on the emission occurring further out. However, the interpretation of the modulation as inverse Compton scattering off stellar photons requires the high-energy electrons to be within the system.
  • 26
    • 72149111875 scopus 로고    scopus 로고
    • note
    • The gamma rays in the Fermi energy range are unaffected by Compton scattering in the stellar wind or by pair production on the stellar UV photons.
  • 27
  • 31
    • 72149106675 scopus 로고    scopus 로고
    • note
    • The Fermi LAT Collaboration acknowledges support from a number of agencies and institutes for both development and the operation of the LAT as well as scientific data analysis. These include NASA and the Department of Energy in the United States; CEA/Institut de Recherches sur les lois Fondamentales de l'Univers and l'Institut National de Physique Nucléaire et de Physique des Particules/CNRS in France; the Agenzia Spaziale Italiana and Istituto Nazionale di Fisica Nucleare in Italy; the Ministry of Education, Culture, Sports, Science and Technology, National Laboratory for High Energy Physics (KEK), and Japan Aerospace Exploration Agency in Japan; and the K. A. Wallenberg Foundation, Swedish Research Council and National Space Board in Sweden. Additional support from the Istituto Nazionale di Astrofisica in Italy and the Centre National d'Etudes Spatiales in France for science analysis during the operations phase is also gratefully acknowledged. J.C. is a Royal Swedish Academy of Sciences Research Fellow, funded by a grant from the K. A. Wallenberg Foundation. G.D. and A.B.H. are funded by contract ERC-StG-200911 from the European Community.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.