The MAIA candidate star HD 208727

Details The MAIA candidate star HD 208727 The MAIA candidate star HD 208727

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...388l..37k&link_type=abstract

Astronomy and Astrophysics, v.388, p.L37-L39 (2002)

Astronomy and Astrophysics

Astrophysics

4

Stars: Variables: General, Stars: Fundamental Parameters: Radii, Stars: Individual: Hd 208727

Scientific paper

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.

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