论文信息 - A Hertzsprung-Russell Diagram For Stellar Oscillations

A Hertzsprung-Russell Diagram For Stellar Oscillations

I present evolutionary tracks and curves of constant central hydrogen abundance in diagrams based on frequencies of high-order, low- degree p modes. For stars with masses between 0.7 and 1.5 M ⨀, a clean separation is obtained between the effects of varying mass and varying evolutionary state.

Jørgen Dalsgaard | Jørgen Dalsgaard

[1] M. Tassoul,et al. Asymptotic approximations for stellar nonradial pulsations , 1980 .

[2] D. Gough. Solar and Solar-Like Oscillations: Theory , 1986 .

[3] Douglas O. Gough,et al. Detection of solar five-minute oscillations of low degree , 1982 .

[4] R. K. Ulrich,et al. Determination of stellar ages from asteroseismology , 1986 .

[5] A. Mangeney,et al. Space research prospects in stellar activity and variability , 1984 .

[6] Jørgen Christensen-Dalsgaard,et al. On solar models and their periods of oscillation , 1982 .