Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...256..107z&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 256, no. 1, p. 107-112.
Astronomy and Astrophysics
Astrophysics
16
Light Curve, Stellar Models, Stellar Oscillations, Variable Stars, Amplitude Distribution Analysis, Electrophotometry, Vibration Mode
Scientific paper
Long series of visual and photoelectric observations of UU Her since 1908 has been analyzed. It is shown that UU Her is a double-mode semiregular variable, the two excited modes of pulsation are probably the fundamental and the first overtone. A simple model is presented to explain the amplitude variations observed in both modes. The model which assumes pure sinusoidal amplitude variation is quite successful in explaining the power spectrum of the variable. The question of the mass of UU Her is also discussed. It is argued that no observation of the star so far points unambiguously to its having a low mass.
Sasselov Dimitar D.
Zsoldos Endre
No associations
LandOfFree
The pulsations of yellow semiregular variables. I - Double-mode behaviour of UU Herculis 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 The pulsations of yellow semiregular variables. I - Double-mode behaviour of UU Herculis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The pulsations of yellow semiregular variables. I - Double-mode behaviour of UU Herculis will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1214033