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Astron. Astrophys. 329, 380 (1998)

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Low-energy line emission from Cygnus X-2 observed
with the BeppoSAX LECS

E. Kuulkers 1, 2, A.N. Parmar 1, A. Owens 1, T. Oosterbroek 1 and U. Lammers 1

1 Astrophysics Division, Space Science Department of ESA, ESTEC, P.O. Box 299, 2200 AG Noordwijk, The Netherlands
2 Astrophysics, University of Oxford, Nuclear and Astrophysics Laboratory, Keble Road, Oxford, OX1 3RH, UK

Astron. Astrophys. 323, L29-L32 (1997)

In the original figure the left hand panel was printed twice. The correct figure is given below.

[FIGURE] Fig. 1. The observed LECS spectrum together with the best-fit cut-off power-law model with the normalization of the 1.02 keV emission feature set to zero (upper left panel). The lower left panel shows the residuals. The right panel shows the inferred photon spectrum and the model prediction including the 1.02 keV feature.

Send offprint requests to: E. Kuulkers: erik@astro.ox.ac.uk

© European Southern Observatory (ESO) 1998

Online publication: November 24, 1997