An asteroseismic membership study of the red giants in three open clusters observed by Kepler: NGC6791, NGC6819, and NGC6811
arXiv:1107.1234 · doi:10.1088/0004-637X/739/1/13
Abstract
Studying star clusters offers significant advances in stellar astrophysics due to the combined power of having many stars with essentially the same distance, age, and initial composition. This makes clusters excellent test benches for verification of stellar evolution theory. To fully exploit this potential, it is vital that the star sample is uncontaminated by stars that are not members of the cluster. Techniques for determining cluster membership therefore play a key role in the investigation of clusters. We present results on three clusters in the Kepler field of view based on a newly established technique that uses asteroseismology to identify fore- or background stars in the field, which demonstrates advantages over classical methods such as kinematic and photometry measurements. Four previously identified seismic non-members in NGC6819 are confirmed in this study, and three additional non-members are found -- two in NGC6819 and one in NGC6791. We further highlight which stars are, or might be, affected by blending, which needs to be taken into account when analysing these Kepler data.
12 pages, 9 figures, 5 tables, accepted by ApJ
References in corpus (11)
- Preparation of Kepler lightcurves for asteroseismic analyses
- Fundamental Properties of Stars using Asteroseismology from Kepler & CoRoT and Interferometry from the CHARA Array
- Asteroseismology of red giants from the first four months of Kepler data: Fundamental parameters
- Asteroseismology of red giants from the first four months of Kepler data: Global oscillation parameters for 800 stars
- The universal red-giant oscillation pattern; an automated determination with CoRoT data
- Sounding open clusters: asteroseismic constraints from Kepler on the properties of NGC 6791 and NGC 6819
- Oscillating K giants with the WIRE satellite: determination of their asteroseismic masses
- Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. I. Measurements, methods, and first results
- High resolution infrared spectroscopy of the old open cluster NGC6791
- Asteroseismic inferences on red giants in open clusters NGC 6791, NGC 6819 and NGC 6811 using Kepler
- Amplitudes of solar-like oscillations: constraints from red giants in open clusters observed by Kepler
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- Uncertainties on near-core mixing in red-clump stars: effects on the period spacing and on the luminosity of the AGB bump
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- WIYN Open Cluster Study. LX. Spectroscopic Binary Orbits in NGC 6819
- The K2 M67 Study: Revisiting old friends with K2 reveals oscillating red giants in the open cluster M67
- Period spacings in red giants IV: Toward a complete description of the mixed-mode pattern
- Searching for Chemical Signatures of Multiple Stellar Populations in the Old, Massive Open Cluster NGC 6791
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- Solar-like oscillations in red giants observed with \textit{Kepler}: influence of increased timespan on global oscillation parameters
- Kepler red-clump stars in the field and in open clusters: constraints on core mixing
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- Testing Asteroseismic Scaling Relations using Eclipsing Binaries in Star Clusters and the Field
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- The Age and Distance of the Kepler Open Cluster NGC 6811 from an Eclipsing Binary, Turnoff Star Pulsation, and Giant Asteroseismology
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- The Gaia-ESO Survey: properties of newly discovered Li-rich giants
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- WIYN Open Cluster Study. LIX. Radial-Velocity Membership of the Evolved Population of the Old Open Cluster NGC 6791
- The K2 M67 Study: An Evolved Blue Straggler in M67 from K2 Mission Asteroseismology
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- Convective-core overshoot and suppression of oscillations: Constraints from red giants in NGC6811
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- Asteroseismology of the Hyades with K2: first detection of main-sequence solar-like oscillations in an open cluster
- Asteroseismology of overmassive, undermassive, and potential past members of the open cluster NGC6791
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- UVIT Open Cluster Study. X. Rich Collection of Post Mass Transfer Systems in NGC 6791
- Planets in Open Clusters Detectable by Kepler
- Vetting Asteroseismic Measurements using Neural Networks
- The Kepler IRIS Catalog: Image subtraction light curves for 9,150 stars in and around the open clusters NGC 6791 and NGC 6819
- Characteristics of solar-like oscillations of secondary red clump stars
- Observational techniques to measure solar and stellar oscillations
- TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting An Extremely Eccentric Exoplanet
- Asteroseismic analysis of eight solar-like oscillating evolved stars in the open cluster NGC 6811
- Asteroseismology of KIC 8263801:Is it a member of NGC 6866 and a red clump star?
- New red giants in NGC 6791 and NGC 6819 using Kepler superstamps
- Stellar oscillations - the adiabatic case
- The odd bunch: chrono-chemo-dynamics of sixteen unusual stars from Kepler
- Kepler Pixel Project -- background RR Lyrae stars in the primary Kepler mission field of view
- Peak Bagging of red giant stars observed by Kepler: first results with a new method based on Bayesian nested sampling