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标题：Probing the shape of the mixing profile and of the thermal structure at the convective core boundary through asteroseismology
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作者：M. Michielsen ; M. G. Pedersen ; K. C. Augustson 等
期刊名称：Astronomy & Astrophysics
印刷版ISSN：0004-6361
电子版ISSN：1432-0746
出版年度：2019
卷号：628
页码：1-11
DOI：10.1051/0004-6361/201935754
语种：English
出版社：EDP Sciences
摘要：Aims.We investigate from a theoretical perspective if space asteroseismology can be used to distinguish between different thermal structures and shapes of the near-core mixing profiles for different types of coherent oscillation modes in massive stars with convective cores; we also examine whether this capacity depends on the evolutionary stage of the models along the main sequence.Methods.We computed 1D stellar structure and evolution models for four different prescriptions of the mixing and temperature gradient in the near-core region. We investigated their effect on the frequencies of dipole prograde gravity modes in slowly pulsating B stars and inβCep stars as well as pressure modes inβCep stars.Results.A comparison between the mode frequencies of the different models at various stages during the main sequence evolution reveals that they are more sensitive to a change in temperature gradient than to the exact shape of the mixing profile in the near-core region. Depending on the duration of the observed light curve, we can distinguish between either just the temperature gradient, or also between the shapes of the mixing coefficient. The relative frequency differences are in general larger for more evolved models and are largest for the higher frequency pressure modes inβCep stars.Conclusions.In order to unravel the core boundary mixing and thermal structure of the near-core region, we must have asteroseismic masses and radii with ∼1% relative precision for hundreds of stars.
关键词：enasteroseismologyconvectionstars: oscillationsstars: interiorsstars: massivetechniques: photometric