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The acoustic spectrum of alpha Cen A

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arxiv astro-ph/0206051 v1 pith:Y37ZCBMB submitted 2002-06-04 astro-ph

The acoustic spectrum of alpha Cen A

classification astro-ph
keywords alphaobservationsspectrumacousticamplitudesanalysisaveragebeen
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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This paper presents the analysis of Doppler p-mode observations of the G2V star $\alpha$ Cen A obtained with the spectrograph CORALIE in May 2001. Thirteen nights of observations have made it possible to collect 1850 radial velocity measurements with a standard deviation of about 1.5 m s$^{-1}$. Twenty-eight oscillation modes have been identified in the power spectrum between 1.8 and 2.9 mHz with amplitudes in the range 12 to 44 cm s$^{-1}$. The average large and small spacing are respectively equal to 105.5 and 5.6 $\mu$Hz. A comparison with stellar models of $\alpha$ Cen A is presented.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. CORALIE radial-velocity search for companions around evolved stars (CASCADES) V. Three planetary companions and achievable precision

    astro-ph.EP 2026-06 conditional novelty 5.0

    Three Jupiter-mass planets are detected around two low-luminosity red giants with 15–18 yr CORALIE RVs; a multi-exposure strategy averages pulsations below 5 m/s.

  2. CORALIE radial-velocity search for companions around evolved stars (CASCADES) V. Three planetary companions and achievable precision

    astro-ph.EP 2026-06 unverdicted novelty 4.0

    Three massive planets detected around HD125136 (2.26 MJup, 850 d) and HD127195 (0.66 and 0.78 MJup, 535 d and 834 d) via Bayesian Keplerian modeling of CORALIE RV series; one additional signal attributed to activity.

  3. Asteroseismology of solar-type stars

    astro-ph.SR 2019-06 unverdicted novelty 2.0

    This review summarizes the development, techniques, and open questions in asteroseismology of solar-type stars whose oscillations are stochastically excited by surface convection.