Current linear structure inversions with mixed modes are unreliable for subgiant stars because the mode kernels change too rapidly with evolution, while main-sequence inversions remain valid.
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Linearity of Structure Kernels in Main-sequence and Subgiant Solar-like Oscillators
Current linear structure inversions with mixed modes are unreliable for subgiant stars because the mode kernels change too rapidly with evolution, while main-sequence inversions remain valid.