X-ray spectral behavior of the relativistic jet source Cygnus X-3

Astrophysical Letters and Communications

Volumn 38, Issue 1-6, 1998, Pages 105-108

  McCollough, M L ^a   Robinson, C R ^a   Zhang, S N ^a   Harmon, B A ^b   Paciesas, W S ^c   Dieters, S ^c   Phengchamnan, S ^c   Hjellming, R M ^d   Rupen, M ^d   Mioduszewski, A J ^d   Waltman, E B ^e   Ghigo, F D ^f   Pooley, G G ^g   Fender, R P ^h   Cui, W ⁱ   Trushkin, S ^j  

^a UNIVERSITIES SPACE RESEARCH ASSOCIATION   (United States)

^b NASA MARSHALL SPACE FLIGHT CENTER   (United States)

^c UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^d NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^e NAVAL RESEARCH LABORATORY   (United States)

^f National Radio Astronomy Observatory NRAO   (United States)

^g CAVENDISH LABORATORY   (United Kingdom)

^h UNIVERSITY OF AMSTERDAM   (Netherlands)

ⁱ MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

^j RUSSIAN ACADEMY OF SCIENCES   (Russian Federation)

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Author keywords

Cygnus X 3; Radio Source; Relativistic Jets; X Ray Binary

Indexed keywords

EID: 33751422663     PISSN: 08886512     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (7)

1. Bonnet-Bidaud, J.M. & Chardin, G. 1988, Physics Reports, 170, 326.
2. McCollough, M.L., et al. 1997a, in "Transparent Universe", ESA, SP-382, p. 263.
3. McCollough, M.L., et al. 1997b, 4th Compton Symposium, (AIP Press) p. 813.
4. McCollough, M.L., et al. 1999, ApJ, accepted.
5. Mioduszewski, A.J. et al. 1998, Proc. of IAU Colloquium 164, 351.
6. Nakamura, H., et al. 1993, MNRAS, 261, 353.
7. Zhang, S. N., et al. 1997, ApJ, 477, L95.