Year: 2007
Type: conference-paper
Abstract: The past few years have seen great progress in observing oscillations in solar‐type stars lying on or just above the main sequence. We review the most recent results, most of which were obtained using high‐precision velocity measurements. We also briefly discuss observations of more evolved stars, namely G, K and M giants and supergiants.
Source: AIP conference proceedings
DOI: 10.1063/1.2818959
Institutions: The University of Sydney, Aarhus University
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W2953088277