000002370 001__ 2370
000002370 005__ 20160701171704.0
000002370 037__ $$aASTROimport-527
000002370 100__ $$aCuypers, J.
000002370 245__ $$aMultiple Periodicity in Pulsating Stars: A Caveat
000002370 260__ $$c1998
000002370 520__ $$aMultiperiodicity is commonly observed in pulsating stars. More and more stars have now already a long series of observations, but high precision photometric and spectroscopic measurements (radial velocity and line profile variations) are in most cases interrupted by long time gaps. The influence of these interruptions on the results of the period analysis is not always taken into account. With the example of the b Cephei star b Crucis, where a lot of a priori information is available, it is shown how the analysis of data with large time gaps can lead to an erroneous set of periods. 
000002370 700__ $$a Minarini, R.
000002370 773__ $$c218$$pA Half Century of Stellar Pulsation Interpretation$$v135$$y1998
000002370 85642 $$ahttp://esoads.eso.org/abs/1998ASPC..135..218C
000002370 905__ $$apublished in
000002370 980__ $$aNONREF