Computer Science
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003javso..31..173p&link_type=abstract
The Journal of the American Association of Variable Star Observers, vol. 31, no. 2, p. 173 (Abstract only)
Computer Science
Rz Aries, V523 Monoceros, Bc Canis Minor, Ux Lynx, Fs Coma Berenices, Red Giants
Scientific paper
We have analyzed the complex variability of five small-amplitude pulsating red giants--RZ Ari, V523 Mon, BC CMi, UX Lyn, FS Com--using a 5000-day database of V photometry from a robotic telescope. For each of these stars, two or three periods recur in each season, and are present in separate halves of the dataset. The periods and their ratios are consistent with low-order radial pulsation modes; the stars are pulsating in multiple overtones, or harmonics. The amplitudes of the modes rise and fall significantly on time scales of 2000 to 3500 days. In UX Lyn and FS Com, there are long secondary periods which add a bass drone to the wavering chord of the radial modes. Even with all these periods accounted for, there are small residuals, which suggest that the celestial harmony is even more complex than we might think.
Bakos Akos G.
Besla Gurtina
Henry Gregory W.
Percy John R.
Velocci Vince
No associations
LandOfFree
Heavenly Harmony: Red Giants Pulsating in Many Modes 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 Heavenly Harmony: Red Giants Pulsating in Many Modes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Heavenly Harmony: Red Giants Pulsating in Many Modes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-882163