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[en] A new X-ray burst source, XB 1715-321, was discovered with the Hakucho satellite. Three type I X-ray bursts were observed from this source in 1979. The error region for XB 1715-321, about 0.3 square degrees in area, includes a persistent X-ray source MX/2S 1715-321 which has been suspected to be the source of several fast transient events. Those bursts detected by Hakucho are characterized by a slow rise time (5--10 s) and a relatively long burst interval
Journal
Astrophysical Journal, Letters to the Editor; ISSN 0571-7248; 
; v. 244(2); p. L79-L83
; v. 244(2); p. L79-L83