activity
20052007
most citedMultisite campaign on the open cluster M67. II. Evidence for solar-like oscillations in red giant stars

64 citations · 141 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph200731 cited

Multisite campaign on the open cluster M67. III. Delta Scuti pulsations in the blue stragglers

H. Bruntt, D. Stello, J. C. Suarez +20

We have made an asteroseismic analysis of the variable blue stragglers in the open cluster M67. The data set consists of photometric time series from eight sites using nine 0.6-2.1…

astro-ph200727 cited

Oscillating Blue Stragglers, gamma Doradus stars and eclipsing binaries in the open cluster NGC2506

T. Arentoft, J. De Ridder, F. Grundahl +9

This is the first step in a project to combine studies of eclipsing binaries and oscillating stars to probe the interior of Blue Stragglers (BS). This may imply a way to discrimina…

astro-ph20071 cited

Solar-like oscillations in open cluster stars

D. Stello, H. Bruntt, T. Arentoft +19

Asteroseismology of stellar clusters is potentially a powerful tool. The assumption of a common age, distance, and chemical composition provides constraints on each cluster member,…

astro-ph200764 cited

Multisite campaign on the open cluster M67. II. Evidence for solar-like oscillations in red giant stars

D. Stello, H. Bruntt, H. Kjeldsen +19

Measuring solar-like oscillations in an ensemble of stars in a cluster, holds promise for testing stellar structure and evolution more stringently than just fitting parameters to s…

astro-ph200618 cited

Multi-site campaign on the open cluster M67. I. Observations and photometric reductions

D. Stello, T. Arentoft, T. R. Bedding +18

We report on an ambitious multi-site campaign aimed at detecting stellar variability, particularly solar-like oscillations, in the red giant stars in the open cluster M67 (NGC 2682…

astro-ph2005

Abundances in giant stars of the globular cluster NGC 6752

David Yong, Frank Grundahl, Poul Erik Nissen +2

Recent theoretical yields and chemical evolution models demonstrate that intermediate-mass AGB stars cannot reproduce the observed abundance distributions of O, Na, Mg, and Al. As…