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2002A&A...388L..37K - Astronomy and Astrophysics, volume 388, L37-39 (2002/6-3)
The MAIA candidate star HD 208727.
KALLINGER T., REEGEN P. and WEISS W.W.
Abstract (from CDS):
HD 208727 is a suspected member of the enigmatic maia variables and shows the largest yet observed amplitude in light variation for any of the potential members. Proven beyond doubt pulsation would pose a serious problem for stellar modelling and opacities, because either opacity source for driving pulsation has to be a different or new identified, yet unkown, pulsation mechanism. We conclude from our investigation that rotation is a more likely explanation for the light variability of HD 208727.
Abstract Copyright: ∼
Journal keyword(s): stars: variables: general - stars: fundamental parameters: radii - stars: individual: HD 208727
Simbad objects: 11
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