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While the bulk of these stars were located in the Orion OB1a and OB1b
fields, two stars of particular interest were monitored from
our Mount Stony Brook Observatory. One of these stars was TAP 26
(NTTS 041559+1716, HBC 376). This star, located in Taurus, had a
measured rotational period which was inconsistent with its 
.
The other star was P1724, located
near Orion OB1d, for which x--ray periodicity had been observed.