Rotational evolution of the Sun

Date

1992-6

Author

Kızıloğlu, N.

Metadata

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The evolutionary behaviour of rotating solar models with different initial angular-momentum distributions has been investigated through the pre-Main-Sequence and Main-Sequence phases. The angular momentum was removed from the convective envelope of the solar models according to the Kawaler's model of magnetic stellar wind (Kawaler, 1988). The models show that (i) the surface rotational velocities of the solar mass stars are independent of initial angular momentum for ages greater than 10(8) years and (ii) it is not possible to explain the neutrino problem and the sufficient depletion of lithium in the Sun.

Subject Keywords

Space and Planetary Science, Astronomy and Astrophysics, Solar-Type Stars, Maın-Sequence Stars

URI

https://hdl.handle.net/11511/52170

Journal

Astrophysics and Space Science

DOI

https://doi.org/10.1007/bf00653263

Collections

Department of Physics, Article

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Citation Formats

N. Kızıloğlu, “Rotational evolution of the Sun,” Astrophysics and Space Science, pp. 83–89, 1992, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/52170.