1. A search for solar-like oscillations in K giants in the globular cluster M4
- Author
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Frandsen, S., Bruntt, H., Grundahl, F., Kopacki, G., Kjeldsen, H., Arentoft, T., Stello, D., Bedding, T. R., Jacob, A. P., Gilliland, R. L., Edmonds, P. D., Michel, E., and Matthiesen, J.
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Astrophysics - Abstract
To expand the range in the colour-magnitude diagram where asteroseismology can be applied, we organized a photometry campaign to find evidence for solar-like oscillations in giant stars in the globular cluster M4. The aim was to detect the comb-like p-mode structure characteristic for solar-like oscillations in the amplitude spectra. The two dozen main target stars are in the region of the bump stars and have luminosities in the range 50-140 Lsun. We collected 6160 CCD frames and light curves for about 14000 stars were extracted. We obtain high quality light curves for the K giants, but no clear oscillation signal is detected. High precision differential photometry is possible even in very crowded regions like the core of M4. Solar-like oscillations are probably present in K giants, but the amplitudes are lower than classical scaling laws predict., Comment: 14 pages, 16 figures, accepted for publication in A&A
- Published
- 2007
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