Convection and Overshoot in Models of Doradus and Scuti Stars
- Mount Allison Univ., Sackville, NB (Canada); Univ. of California, Santa Barbara, CA (United States). Kavli Inst. for Theoretical Physics
- Univ. of California, Santa Barbara, CA (United States). Kavli Inst. for Theoretical Physics; Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
We investigate the pulsation properties of stellar models that are representative of δ Scuti and γ Doradus variables. Here we have calculated a grid of stellar models from 1.2 to 2.2 M ⊙, including the effects of both rotation and convective overshoot using MESA, and we investigate the pulsation properties of these models using GYRE. We discuss the observable patterns in the frequency spacing for p modes and the period spacings for g modes. Using the observable patterns in the g mode period spacings, it may be possible to observationally constrain the convective overshoot and rotation of a model. We also calculate the pulsation constant (Q) for all models in our grid and investigate the variation with convective overshoot and rotation. The variation in the Q values of the radial modes can be used to place constraints on the convective overshoot and rotation of stars in this region. Finally, as a test case, we apply this method to a sample of 22 High-Amplitude δ Scuti stars (HADS) and provide estimates for the convective overshoot of the sample.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- USDOE National Nuclear Security Administration (NNSA), Office of Defense Programs (DP)
- Grant/Contract Number:
- AC52-06NA25396
- OSTI ID:
- 1407896
- Report Number(s):
- LA-UR-17-25700; TRN: US1702927
- Journal Information:
- The Astrophysical Journal (Online), Vol. 849, Issue 1; ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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