Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

Bedding, T. R. (2011). Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars. Nature, 608-611.

Type

Journal article

Intellectual base

Primary research

Year

2011

Pages

608-611

DOI

10.1038/nature09935

DOI registrant

Springer Nature

Link

https://orbi.uliege.be/bitstream/2268/107456/1/bedding-nature.pdf

Cited by

1 citation across 1 artifact.

Domain-specific

• Solar-Like Oscillations
  • A frequency comb, a broad hump of oscillation power, and finite-width peaks are useful ways to recognize and analyze the regime when the data resolve them; none guarantees that every mathematically available mode or every convective star will be observed.

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