Red-giant seismic properties analyzed with CoRoT

TL;DR

This study analyzes over 4,600 CoRoT light curves of red giants to extract seismic parameters, derive stellar properties, and compare populations, demonstrating the power of statistical asteroseismology in understanding stellar evolution.

Contribution

It provides a large-scale, unbiased analysis of red-giant seismic properties and validates scaling relations for stellar parameter inference from asteroseismic data.

Findings

Identified over 1,800 red giants in the sample.

Derived accurate distributions of stellar mass and radius.

Compared stellar populations from two different Galactic regions.

Abstract

The CoRoT 5-month long observation runs give us the opportunity to analyze a large variety of red-giant stars and to derive fundamental stellar parameters from their asteroseismic properties. We perform an analysis of more than 4\,600 CoRoT light curves to extract as much information as possible. We take into account the characteristics of the star sample and of the method in order to provide asteroseismic results as unbiased as possible. We also study and compare the properties of red giants of two opposite regions of the Galaxy. We analyze the time series with the envelope autocorrelation function in order to extract precise asteroseismic parameters with reliable error bars. We examine first the mean large frequency separation of solar-like oscillations and the frequency of maximum seismic amplitude, then the parameters of the excess power envelope. With the additional information of the effective temperature, we derive the stellar mass and radius. We have identified more than 1\,800 red giants among the 4\,600 light curves and have obtained accurate distributions of the stellar parameters for about 930 targets. We were able to reliably measure the mass and radius of several hundred red giants. We have derived precise information on the stellar population distribution and on the red clump. Comparison between the stars observed in two different fields shows that the stellar asteroseismic properties are globally similar, but with different characteristics for red-clump stars. This study shows the efficiency of statistical asteroseismology: validating scaling relations allows us to infer fundamental stellar parameters, to derive precise information on the red-giant evolution and interior structure and to analyze and compare stellar populations from different fields.