During the Hakucho observations of the galactic center region in 1980 July-August, 15 X-ray bursts were observed for the first time from a bright bulge source GX 3+1 (4U 1744-26). These bursts exhibit characteristics typical of type 1 cosmic X-ray bursts. No bursts, however, were observed from GX 3+1 in previous Hakucho observations conducted in 1979 and early 1980. The persistent X-ray flux of GX3+1 in 1979-1980 was roughly half the value obtained in 1971-1978 by other observers.
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Makishima et al. (1983) studied this question.
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