Abstract
The strongest data supporting this stream’s existence comes from three radar studies conducted during the 1960s. During 1961 June 13–19, C. S. Nilsson (1964) used the equipment at the University of Adelaide (South Australia, Australia) and detected four meteors from α = 293.9°, δ = −8.4°.1 A second radar survey was conducted at Adelaide by G. Gartrell and W. G. Elford (1975) during 1969 June. Thirteen meteors were detected from an average radiant at α = 289°, δ = −6° centered on June 11.2 Finally, during 1969 June 2 to July 2, Z. Sekanina said the Radio Meteor Project at Havana, Illinois (USA) detected 35 meteors. At the time of its nodal crossing on June 17.5 (λ = 85.8°), the radiant was at α = 297.1°, δ = −7.1°.
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