Search for new pulsating O VI central stars of planetary nebulae
Silvotti, R. · Bartolini, C. · Stanghellini, L.
Original · EN
A photoelectric monitoring program has been applied, during the last four years, to five central stars of planetary nebulae (PNNs) with strong OVI λ 3811--34 Å0.1mm emission. NGC6905 and, marginally, NGC2452, show intrinsic luminosity variations, while NGC7026, IC2003 and NGC1501 have constant luminosity within a few mmag. Photometric data have been analyzed with the best available packages for power--spectra reductions. Both pulsators have periods and physical characteristics well encompassed by the theoretical pulsational models relative to these stars.
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