Microvariability in High Amplitude Delta Scuti stars

Details Microvariability in High Amplitude Delta Scuti stars Microvariability in High Amplitude Delta Scuti stars

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996dssn...10...10g&link_type=abstract

Delta Scuti Star Newsletter, Issue 10, p. 10

Physics

Scientific paper

It has been recently pointed out by Walraven et al. (1992) that the Delta Scuti star AI Vel could be oscillating at the mmag level with more periods than the fundamental radial and the first overtone, as was assumed until now. However, the reality of these new periods should be taken with caution because of their low amplitudes. The amplitudes are not only low (a few millimags), but in the frequency range under investigation they are difficult to distinguish from the many frequencies which may be excited by non-linear coupling of the two large-amplitude radial modes. The detection of new periodicities is critically dependent on the photometric quality of the data. Fortunately we have an advantage in the case of the HADS stars: the non-linear interactions of the new frequencies with the radial high-amplitude ones.

Affiliated with

Also associated with

No associations

Rating

Microvariability in High Amplitude Delta Scuti stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Microvariability in High Amplitude Delta Scuti stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Microvariability in High Amplitude Delta Scuti stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1213030