Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2011-08-29
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
To appear in the Carnegie Observatories Astrophysics Series, volume 5
Scientific paper
This paper summarizes the main results of our recent study of the non-Blazhko RR Lyrae stars observed with the Kepler space telescope. These stars offer the opportunity for studying the stability of the pulsations of RR Lyrae stars and for providing a reference against which the Blazhko RR Lyrae stars can be compared. Of particular interest is the stability of the low-dispersion (sigma < 1mmag) light curves constructed from ~18,000 long-cadence (30-min) and (for FN Lyr and AW Dra) the ~150,000 short-cadence (1-min) photometric data points. Fourier-based [Fe/H] values and other physical characteristics are also derived. When the observed periods are compared with periods computed with the Warsaw non-linear convective pulsation code better agreement is achieved assuming pulsational L and M values rather than the (higher) evolutionary L and M values.
Benkö József M.
Borucki William. J.
Bryson Stephen
Caldwell Doug
Chadid Merieme
No associations
LandOfFree
Non-Blazhko RR Lyrae Stars Observed with the KEPLER Space Telescope 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 Non-Blazhko RR Lyrae Stars Observed with the KEPLER Space Telescope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-Blazhko RR Lyrae Stars Observed with the KEPLER Space Telescope will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-127146