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Astron. Astrophys. 325, 1283 (1997)

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Discovery of an unusual new superoutburst star in Aquarius. Is it a superflare star or a fast nova?

I. Toth , S. Barcza and A. Frontó

Konkoly Observatory, Budapest H-1525, P.O. Box 67, Hungary

Astron. Astrophys. 315, 153--159 (1996)

On page 158 the second sentence of the second paragraph is slightly erroneous. It should read:

Moreover, on the time scale of 40 days the novae generally have amplitudes of 6 mag, except for V1500 Cyg (1975) (Duerbeck 1981) and CP Pup (1942) (Pettit 1954) which had about 10-13 mag outburst amplitude.

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© European Southern Observatory (ESO) 1997

Online publication: April 28, 1998