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Radio-X-Ray Connection for X-Ray Transients and Binaries

Published online by Cambridge University Press:  14 August 2015

R.M. Hjellming
R.M. Hjellming*
Affiliation:
National Radio Astronomy Observatory†, Socorro, NM 87801USA

Extract

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The discovery of the association between relativistic radio jets and X-ray events in GRS 1915+105 (Mirabel and Rodriguez, 1994) and GRO J1655-40 showed that strong radio flares (Harmon et al, 1994) in general, and jet ejection (Hjellming and Rupen, 1994) in particular, could be identified with features in hard X-ray events. This has caused us to re-think the interpretation of the radio events in X-ray transients, and has made multi-wavelength observations even more important. In this paper the focus is on the connection between X-ray and radio events as seen since 1994 in GRS 1915+105, GRO J1655-40, GRO J1719-24, GRO J1739-278, Cyg X-3, Cyg X-l, and Sco X-l.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 11 , Issue 2: Highlights of Astronomy. As presented at the XXIIIrd General Assembly of the IAU (Part B), 1997 , 1998 , pp. 767 - 770
Copyright
Copyright © Kluwer 1998

References

Ball, L. et al. (1995), M.N.R.A.S., 273, pp. 722–730 Google Scholar
Blandford, R. and Payne, D.G. (1982), M.N.R.A.S., 199, pp. 883–903 CrossRefGoogle Scholar
Davis, R.J. et al. (1975), Nature, 257, p. 659 Google Scholar
Han, X. and Hjellming, R.M. (1992), Ap.J., 400, pp. 304–314 CrossRefGoogle Scholar
Harmon, B.A. et al. (1995), Nature, 374, pp. 703–706 Google Scholar
Hjellming, R.M. (1997), In Accretion Phenomena and Related Outflows, PASP Conference Proc, 121, Ed. Wickramasinghe, D.T., Bicknell, G.V., & Ferrario, L., pp. 53–62 Google Scholar
Hjellming, R.M. & Johnston, K.J. (1981), Ap.J., 246, pp. L141–L144 Google Scholar
Hjellming, R. M. & Rupen, M. P. (1995), Nature, 375, pp. 464–468 Google Scholar
Hjellming, R.M., et al. (1988), Ap.J., 335, pp. L75–L78 Google Scholar
Hjellming, R.M., et al. (1996), Ap.J., 470, pp. L105–L107 Google Scholar
Hunstead, R.W., Wu, K., and Campbell-Wilson, D. (1997), In Accretion Phenomena and Related Outflows, PASP Conference Proc, 121, Ed. Wickramasinghe, D.T., Bicknell, G.V., & Ferrario, L., pp. 63–67 Google Scholar
Kotani, T. et al. (1996), P.A.S.J., 48, pp. 619–629 Google Scholar
McCullough, et al. (1997), In The Transparent Universe, ESA SP-382, pp. 265–268 Google Scholar
Margon, B. (1984), Ann. Rev. Astron. Astrophys., 22, pp. 507–536 Google Scholar
Meier, D.L. (1997), In Accretion Phenomena and Related Outflows, PASP Conference Proc, 121, Ed. Wickramasinghe, D.T., Bicknell, G.V., & Ferrario, L., pp. 68–71 Google Scholar
Meier, D.L. et al, (1997), Nature, 388, pp. 350–352 Google Scholar
Mioduszewski, A.J. et al. (1997), Proceedings of IAU Colloquium 183, P.A.S.P. Conference Series, Ed. Zensus, A., Wrobel, J., & Taylor, G.B., in pressGoogle Scholar
Mirabel, I. F. & Rodriguez, L. F. (1994), Nature, 371, pp. 46–48 CrossRefGoogle Scholar
Narayan, R. (1997), In Accretion Phenomena and Related Outflows, PASP Conference Proc, 121, Ed. Wickramasinghe, D.T., Bicknell, G.V., & Ferrario, L., pp. 75–89 Google Scholar
Owen, F.N. et al. (1976), Ap.J., 203, pp. L15–L16 Google Scholar
Robinson, C.R.. et al. (1998), in preparation.Google Scholar
Schrader, C.R. et al. (1994), Ap.J., 434, pp. 698–706 Google Scholar
Tingay, J. et al. (1995), Nature, 374, pp. 141–143 Google Scholar
Vermeulen, R.C. 1989, Multiwavelength Studies of SS433, Ph.D. Thesis, Rijksnunversiteit Leiden, Netherlands.Google Scholar
Vermeulen, R.C. et al. (1987), Nature, 328, pp. 309–313 Google Scholar
Watson, M.G. et al. (1986), M.N.R.A.S., 222, pp. 261–271 Google Scholar
Zhang, N. et al. (1997), Ap.J., 477, pp. L95–L98 CrossRefGoogle Scholar