We recently reported strong evidence for solar-like oscillations in the G0 IV star η Boo (Kjeldsen et al. 1995, AJ 109, 1313). We measured small temperature fluctuations produced by oscillations through their effect on the equivalent widths of the Balmer lines. Here we address several issues that were raised at this conference.
No takes yet. Share an insight, caveat, or question.
Bedding et al. (1995) studied this question.
Synapse has enriched 5 related papers. Consider them for comparative context: