Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...264..138p&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 264, no. 1, p. 138-146.
Astronomy and Astrophysics
Astrophysics
25
Helioseismology, Stellar Cores, Stellar Evolution, Stellar Oscillations, Fabry-Perot Interferometers, Hertzsprung-Russell Diagram, P Waves, Power Spectra
Scientific paper
This paper reports the results of an attempt to measure solar-like p-modes of oscillation on Alpha Cen A, using a carefully stabilized Fabry-Perot velocity analyzer. Detection of individual modes of oscillation near 5 min period is proposed, based on the comb-like signature which is similar to that found in the sun. The mean peak amplitudes of the strongest individual modes are in the range of 75 to 120 cm/s, and the mean separation between alternate modes is 55.3 +/- 3.6 micro-Hz. Apparent modal lifetimes are on the order of 2 days, but we suggest this may be caused by interference of adjacent modes. A preliminary discussion of the evolutionary state of Alpha Cen A is made based on these observations.
Butcher Harvey R.
Pottasch Edward M.
van Hoesel Frans H. J.
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