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Radio, Infrared and X-Ray Observations of GRS 1915+105

Published online by Cambridge University Press:  12 April 2016

R.P. Fender ,
G.G. Pooley ,
C.R. Robinson ,
B.A. Harmon ,
S.N. Zhang  and
C. Canosa
R.P. Fender
Affiliation:
Astronomy Centre, University of Sussex, Brighton BN1 9QH, U.K.
G.G. Pooley
Affiliation:
MRAO, Cavendish Laboratory, Cambridge CBS OHE, U.K.
C.R. Robinson
Affiliation:
MSFC, Huntsville, AL 35812, U.S.A.
B.A. Harmon
Affiliation:
MSFC, Huntsville, AL 35812, U.S.A.
S.N. Zhang
Affiliation:
MSFC, Huntsville, AL 35812, U.S.A.
C. Canosa
Affiliation:
Astronomy Centre, University of Sussex, Brighton BN1 9QH, U.K.

Abstract

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We present multiwavelength observations of the superluminal jet source GRS 1915+105 in 1996 April–May, over which period a variety of phenomena, including radio QPO, strong infrared emission lines and rapid X-ray flickering and outbursts were observed.

Type
Part 15. Poster Papers
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 701 - 702
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Castro-Tirada, A.J. et al. 1996, ApJ, 461, L99 Google Scholar
Foster, R.S. et al. 1996, ApJ, 467, L81 CrossRefGoogle Scholar
Mirabel, I.F., Rodriguez, L.F. 1994, Nature, 371, 46 CrossRefGoogle Scholar