Seismic Diagnostics of Mixing Beyond the Convective Core in Intermediate Mass Main-Sequence Stars

• Autorzy: Popielski, B. L. , Dziembowski, W. A.
• Języki publikacji: EN

Abstrakty

EN

We study prospects for seismic sounding the layer of a partial mixing above the convective core in main-sequence stars with masses in the 1.2-1.9 M_solar range. There is an initial tendency to increase of the convective core mass in such stars and this leads to ambiguities in modeling. Solar-like oscillations are expected to be excited in such objects. Frequencies of such oscillations provide diagnostics, which are sensitive to the structure of the innermost part of the star and they are known as the small separations. We construct evolutionary models of stars in this mass range assuming various scenarios for element mixing, which includes formation of element abundance jumps, as well as semiconvective and overshooting layers. We find that the three point small separations employing frequencies of radial and dipole modes provide the best probe of the element distribution above the convective core. With expected accuracy of frequency measurement from the space experiments, a discrimination between various scenarios should be possible.

Słowa kluczowe

EN

stars: oscillations; stars: evolution; convection

• Czasopismo: Acta Astronomica
• Rocznik: 2005
• Tom: Vol. 55, No. 2
• Strony: 177--193
• Opis fizyczny: Bibliogr. 24 poz., tab., wykr.

Twórcy

autor

Popielski, B. L.

• Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland,

autor

Dziembowski, W. A.

• Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warsaw, Poland,
• Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warsaw, Poland

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