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Solar-like Oscillations: An Observational Perspective

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arxiv 1107.1723 v1 pith:PWCGOFGX submitted 2011-07-08 astro-ph.SR

Timothy R. Bedding This is my paper · ORCID
classification astro-ph.SR
keywords oscillationssolar-likeconvectiongiantsmainobservationalsomestars
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Solar-like oscillations are excited stochastically by convection. They occur in stars with an outer convection zone, which includes the Sun and other stars on the lower main sequence, as well as cool subgiants and red giants. This chapter reviews the basic properties of solar-like oscillations and summarises some of the main observational results. Mixed modes in subgiants and red giants are discussed in some detail, including an introduction to the so-called p-g diagram for avoided crossings.

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Cited by 1 Pith paper

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  1. Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS

    astro-ph.SR 2025-05 conditional novelty 5.0 of 10

    Simultaneous SONG radial velocities and TESS photometry of the subgiant beta Aql yield a photometry-to-velocity amplitude ratio of 26.6 +/- 3.1 ppm/(m/s) and an intensity-velocity phase shift of -113 +/- 7 degrees, bo...

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