Astron. Astrophys. 355, L35-L38 (2000)

Footnotes

1. As for V346 Ori and AK Sco, the variation seems Scuti-like, with u amplitudes of about 0.035 and 0.08 mag respectively but no period could be derived due to the poor phase coverage. As for BF Ori, its variation is clear ( 0.11 mag), but seems rather monotonic

© European Southern Observatory (ESO) 2000

Online publication: March 21, 2000
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